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Author SHA1 Message Date
John Tramm
54b661d39f
MGXS Bootstrapping (#3965)
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Co-authored-by: John Tramm <jtramm@gmail.com>
Co-authored-by: Claude Opus 4.8 <noreply@anthropic.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-07-22 05:38:20 +00:00
Satoshi Misumi
852f92780c
Fix M_PI being unavailable where _USE_MATH_DEFINES comes too late (#4023)
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Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-07-21 15:45:41 +00:00
GuySten
61c8a59cff
Override NJOY default damage energy threshold (#4022)
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Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-07-20 14:52:30 +00:00
Mazeyar Moeini Feizabadi
05d01274a7
Add analytic tests for ray-traced intersection distances (#4014)
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2026-07-19 14:49:48 -05:00
Joffrey Dorville
db673b9acb
Automatic C++ doc generation (#3950)
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Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-07-17 15:47:40 +00:00
GuySten
796ae384b8
Fix not reseting filter_matches corrupt pulse height results (#4019)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-07-17 13:18:53 +00:00
GuySten
d3bc1669d3
Access element subshell map data only if it has atomic relaxation data (#4020) 2026-07-17 07:40:16 -05:00
Paul Romano
f1fb6721f0
Performance optimizations for shared secondary bank (#4011)
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2026-07-17 01:25:18 +00:00
Ethan Peterson
c55c578812
Native parametric tokamak source (#3999)
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Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-07-16 09:54:56 -05:00
Paul Romano
16cde42ff4
Enable parent-nuclide tally breakdowns in R2S calculations (#4013)
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Co-authored-by: GuySten <62616591+GuySten@users.noreply.github.com>
2026-07-16 00:00:42 +03:00
Lewis Gross
243c249533
normalize new_u after periodic crossing to prevent unnormalized direction (#4015)
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2026-07-15 08:57:53 -05:00
Eden
e783e01471
Add chain parameter to Material.get_activity for half-life data (#3957)
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Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-07-11 06:18:26 +00:00
Jonathan Shimwell
7256d5046a
extra checks for pixels (#4009)
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Co-authored-by: Jonathan Shimwell <jon@proximafusion.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-07-10 15:02:14 +00:00
Paul Romano
216651b69e
Shared secondary bank performance optimizations (#3995) 2026-07-10 09:22:16 -05:00
Paul Romano
7c408f6a10
Replace Ben Forget with John Tramm on technical committee (#4008)
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2026-07-10 09:48:11 +02:00
Paul Romano
3c3ebba98b
Turn on weight windows if weight_windows_file is specified (#4007)
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2026-07-09 23:59:33 +00:00
GuySten
e73d8048da
Support cell densities per instances in plots (#4006)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-07-09 22:45:09 +00:00
Jonathan Shimwell
5203640549
Further input validation for plot methods (#4004) 2026-07-09 16:55:32 -05:00
Paul Romano
3cdb67e50d
Store slice overlap indices in cell ID field (#4002)
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2026-07-09 11:47:55 +02:00
Paul Romano
8b15ee3915
Add Jon Shimwell to technical committee (#4001)
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2026-07-08 11:25:21 -05:00
Andrew Davis
8684506269
This fixes compile isuees found with GCC 16.1.1 and FMT version (#4000)
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Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-07-07 14:58:19 +00:00
viktormai
0c6b3fb835
Overlap detection for plotter (#3969)
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Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-07-06 17:47:22 +00:00
Paul Romano
3fcb9692be
Make sure output is treated consistently in R2SManager (#3994)
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2026-07-04 22:20:03 -05:00
Matteo Zammataro
e3bc615172
Fix numerical cancellation in RectLattice::distance for large pitch values (#3853)
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Co-authored-by: matteo.zammataro <matteo.zammataro@newcleo.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-07-03 21:39:17 +00:00
Paul Romano
66359e5dd8
Fix surface tally crash on lattice crossings (#3993)
Co-authored-by: GuySten <guyste@post.bgu.ac.il>
2026-07-03 15:52:19 -05:00
Matteo Zammataro
97e04c464a
Add ambient dose coefficients (H*(10)) from ICRP74 (#3256)
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Co-authored-by: matteo.zammataro <matteo.zammataro@newcleo.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-07-02 23:51:10 +00:00
Jon Shimwell
df6f94300f
Turn the weight window game off for a zero or negative lower bound (#3990)
Co-authored-by: John Tramm <john.tramm@gmail.com>
Co-authored-by: shimwell <mail@jshimwell.com>
2026-07-02 13:04:02 -05:00
Paul Romano
3247587d49
Ensure photon cross sections are loaded when FileSource contains photons (#3988)
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2026-07-02 11:54:12 -05:00
John Tramm
24fdb84edc
Tally 32-bit Overflow Fix (#3960)
Co-authored-by: Claude Opus 4.8 (1M context) <noreply@anthropic.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-07-02 11:53:49 -05:00
John Tramm
f01852411d
Random Ray Forward Flux Save in Adjoint Mode (#3962)
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Co-authored-by: Claude Opus 4.8 (1M context) <noreply@anthropic.com>
2026-07-01 22:35:27 +02:00
Jonathan Shimwell
d06fdee93a
Preserve user material names in convert_to_multigroup and avoid overwriting material with same name bug fix (#3984)
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2026-06-30 09:38:09 -05:00
GuySten
4d6244d93c
Fix for numpy 2.5.0 (#3981)
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2026-06-24 16:09:16 -05:00
Paul Romano
608a1c3386
Fix several issues related to independent operator depletion (#3977)
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2026-06-23 09:00:47 +02:00
stetsonschott
09ee8308d0
Replaced 'C0' by elemental carbon in `openmc/examples.py'. (#3974)
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2026-06-17 20:33:40 -05:00
GuySten
02eb999af1
fix tmate start only on successful tests (#3954)
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2026-06-08 22:09:25 -05:00
Logan Harbour
998565808e
Use non-deprecated methods for getting libMesh node points (#3963) 2026-06-08 22:07:21 -05:00
Patrick Shriwise
ea6ba328c9
Fix collision track feature for photon transport (#3946)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-06-08 23:37:34 +00:00
Paul Romano
4f6a25e00a
Introduce new C API function for slice plots (#3806)
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2026-06-08 21:08:08 +00:00
Paul Romano
db322f2c5d
Add section in depletion user's guide about comparing to other codes (#3955) 2026-06-08 18:22:32 +00:00
EdenRochmanSharabi
111eb77066
Implement SphericalMesh.get_indices_at_coords (#3919)
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Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-05-30 06:18:09 +00:00
Jonathan Shimwell
219d82726f
Allow tracklength estimator for neutron heating (#3915)
Co-authored-by: Jon Shimwell <jon@proximafusion.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-05-30 06:10:05 +00:00
hugo-barthod
2dd5322fee
Fix undefined variable in openmc.mgxs.library (scatt_mgxs) (#3943)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-05-30 05:35:31 +00:00
Bor Kos
46d8896132
Pulsed Height Tally in mixed neutron-gamma fields (#3937)
Co-authored-by: Bor Kos <bor.kos@bakerhughes.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-05-30 03:25:38 +00:00
Jon Shimwell
ddabe1c8c5
Avoid storing inconsistent sum/sum_sq on summed D1S tallies (#3949)
Co-authored-by: shimwell <mail@jshimwell.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-05-30 03:25:22 +00:00
Paul Romano
1914e3eefa
Support endf.Material in from_endf methods (#3932) 2026-05-29 21:53:45 -05:00
Ahnaf Tahmid Chowdhury
dfb6c5699c
Modernize CMake packaging (#3653)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-05-21 20:33:56 +00:00
Patrick Shriwise
7d09a12606
DAGMC Cell Override Updates (#3888)
Co-authored-by: Claude Sonnet 4.6 <noreply@anthropic.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-05-20 21:43:21 +00:00
Patrick Shriwise
66497e76b1
Support writing of hex elements to VTKHDF format. (#3623)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-05-20 14:01:21 -05:00
Hridoy Kabiraj
3c7a030d43
Guard average molar mass and validate materials depletion inputs (#3941) 2026-05-20 13:49:00 -05:00
John Tramm
0169fd9226
Shared Secondary Particle Bank (#3863)
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Co-authored-by: Claude Opus 4.6 <noreply@anthropic.com>
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Co-authored-by: Copilot <copilot@github.com>
2026-05-19 23:23:10 -05:00
charliesheh
beed56e6ee
Check for missing thread count argument for -s/--threads (#3940) 2026-05-18 13:35:56 -05:00
Hridoy Kabiraj
195dff6d1d
Fix missing volume checks in material activity/decay heat (#3939) 2026-05-18 09:20:59 -05:00
Paul Romano
d56cda2544
Implement DecaySpectrum distribution type and utilize in R2S (#3930)
Co-authored-by: Copilot <copilot@github.com>
2026-05-08 20:53:12 -05:00
Paul Romano
f3e1066d46
Include mass_attenuation.h5 in package data (#3936) 2026-05-07 23:50:23 +00:00
Jonathan Shimwell
e542b2f035
Allow Mesh.volumes property for 1D and 2D RegularMesh (#3914) 2026-05-06 10:07:35 -05:00
Jack Fletcher
368ea069ca
Local adjoint source for Random Ray (#3717) 2026-04-28 16:10:03 -05:00
Paul Romano
1116c4bdc0
Support multiple meshes in R2S calculations (#3860) 2026-04-28 10:02:08 -04:00
Travis L.
806fb4ce77
Clean up MCPL references (#3927) 2026-04-27 09:40:44 -05:00
Perry
2d5c50080c
Allow the use of substeps for CRAM (#3908)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-04-22 18:24:34 -05:00
Perry
1f7ac4215f
Clip negative atom densities that result from CRAM (#3879)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-04-21 20:24:53 +00:00
Ethan Peterson
a1df5842e0
Remove self loops from spontaneous fission decay mode (#3907)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-04-21 16:47:40 +00:00
Lorenzo Chierici
e431d49bec
Add reactivity control to coupled transport-depletion analyses (#2693)
Co-authored-by: Andrew Johnson <drewejohnson@users.noreply.github.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-04-20 07:13:53 -05:00
Luke Labrie-Cleary
36e70d8efc
Add Arch Linux User Repository (AUR) installation instructions to documentation (#3921)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-04-18 16:01:09 +00:00
Paul Romano
fd1bc26af0
Pin NJOY version in Dockerfile (#3920) 2026-04-09 23:13:18 +03:00
Paul Romano
1eb368bbd2
Pin NJOY version in CI to 2016.78 (#3917) 2026-04-09 09:31:27 +02:00
Paul Romano
23e8a11102
Update versions of several GHA Actions (#3913) 2026-04-05 14:04:34 -05:00
Jonathan Shimwell
542f949fa0
Use local variable to avoid attribute lookup in form_rxn_matrix loop (#3884)
Co-authored-by: Perry <yrrepy@users.noreply.github.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-04-04 20:53:50 +00:00
GuySten
efc542825e
Add the ability to tally microscopic cross sections in void materials with tracklength estimator (#3771)
Co-authored-by: Jonathan Shimwell <drshimwell@gmail.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-04-04 20:32:51 +00:00
Ethan Peterson
60d1dfba7f
Refactor form_matrix method on depletion chain class (#3892)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-04-03 21:27:39 +00:00
John Tramm
b215f13218
RAG search tool for agents (#3861)
Co-authored-by: John Tramm <jtramm@gmail.com>
Co-authored-by: Claude Opus 4.6 <noreply@anthropic.com>
2026-04-03 16:18:19 -05:00
Jonathan Shimwell
9ff50499e1
Adding per m3 to material functions (#3912)
Co-authored-by: Jon Shimwell <jon@proximafusion.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-04-03 00:00:02 +00:00
bessemoa
df985e10b3
Add from_bounding_box classmethod to structured mesh classes (#3903)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-04-02 22:51:33 +00:00
Jonathan Shimwell
ca22a5174a
adding pdf to read the docs (#3893) 2026-04-02 17:01:30 -05:00
GuySten
d9b30bbbd5
Approximate multigroup velocity (#3766)
Co-authored-by: Adam Nelson <1037107+nelsonag@users.noreply.github.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-04-02 16:59:02 +00:00
Md. Ariful Islam
97d9a839c2
Fix MPI depletion hang (#3910) 2026-04-02 11:30:09 -05:00
April Novak
8223099ed9
All reduce to print correct number of surface source particles (#3901) 2026-03-26 12:35:12 -05:00
GuySten
6cd39073b3
Fix surface tally when crossing lattice (#3895) 2026-03-23 10:16:59 -05:00
Paul Romano
3ce6cbfdda
Add fusion_neutron_spectrum to openmc.stats module (#3862) 2026-03-17 22:10:18 +01:00
itay-space
1578698129
Implement angular PDF evaluation for angle-energy distributions (#3550)
Co-authored-by: Your Name <you@example.com>
Co-authored-by: GuySten <62616591+GuySten@users.noreply.github.com>
Co-authored-by: GuySten <guyste@post.bgu.ac.il>
Co-authored-by: Eliezer214 <110336440+Eliezer214@users.noreply.github.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-03-14 23:58:17 +02:00
Marco De Pietri
bc9c31e0f9
get indices for rectilinear meshes (#3876)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-03-14 04:19:51 +00:00
Paul Wilson
dd6d31bfae
Add properties to settings w/ documentation, c++ loading of filename, and python round-trip test (#3808)
Co-authored-by: Patrick C Shriwise <pshriwise@gmail.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-03-13 21:40:52 +00:00
AlvaroCubi
4bda85f17e
Allow StepResult.get_material to accept integer material ID (#3872)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-03-12 15:04:42 -05:00
Christopher Ashe
c44d2f0b43
Allow groups to be passed as sequence of floats in convert_to_multigroup (#3873)
Co-authored-by: Jonathan Shimwell <drshimwell@gmail.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-03-12 19:47:47 +00:00
Paul Romano
27522fe851
Improve review skill instructions for determining PR context (#3875) 2026-03-12 14:27:00 -05:00
CoronelBuendia
387b41ab65
Change plotting docstring to specify integer RGB values (#3868) 2026-03-12 12:35:10 -05:00
Eshed Magali
ba94c58230
Closing the stdout file descriptor when finished (#3864) 2026-03-11 16:50:58 +00:00
Amanda Lund
1dc4aa9882
Add setting to optionally disable atomic relaxation (#3855)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-03-10 04:00:10 +00:00
Paul Romano
908e63115a
Add reusable reviewing-openmc-code skill and Copilot Review agent (#3842)
Co-authored-by: John Tramm <john.tramm@gmail.com>
2026-03-05 21:40:36 -06:00
GuySten
be4148ad0d
Refactor Ray class into its own file (#3845)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-03-06 01:07:42 +00:00
Paul Romano
6f72619729
Fix include guard in output.h (#3856) 2026-03-05 23:29:36 +00:00
John Tramm
533f09defd
Enable CMake "compile_commands.json" Output (#3854)
Co-authored-by: John Tramm <jtramm@gmail.com>
Co-authored-by: Claude Opus 4.6 <noreply@anthropic.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-03-05 23:20:54 +00:00
Paul Romano
dbfd6387b2
Fix two docstrings that should have r prefix (#3851) 2026-03-05 07:37:47 +02:00
Ethan Peterson
2bd06660c5
Parallelize sampling external sources and threadsafe rejection counters (#3830)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-03-04 14:36:43 -06:00
GuySten
0ab46dfa35
Fix cell data parsing (#3848) 2026-03-04 06:56:49 -06:00
GuySten
70be650003
Implement surface flux tallies (#3742)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-03-04 14:17:48 +02:00
Patrick Shriwise
b796afb591
Correction to surface normal determination in SolidRayTrace plots (#3846) 2026-03-04 14:10:54 +02:00
Marco De Pietri
53d98ce71a
Add method on Material for computing photon contact dose rate (#3700)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-03-03 15:48:56 +00:00
Paul Romano
49b896b0eb
Enable "hybrid" tallies in get_microxs_and_flux (#3831) 2026-03-02 22:06:52 -05:00
GuySten
823b4c96c9
Speed up depletion with transfer rates (#3839) 2026-03-02 06:53:20 -06:00
Paul Romano
83a7b36add
Speed up Docker build (#3841)
Co-authored-by: Jonathan Shimwell <drshimwell@gmail.com>
2026-03-01 21:52:51 +02:00
Paul Romano
b3788f11e1
Use clang-format version 18 for CI format checks (#3840) 2026-02-27 13:56:00 +02:00
Micah Gale
1d9a8f542b
Add Python 3.14 to testing matrix and drop Python 3.11 (#3642)
Co-authored-by: GuySten <guyste@post.bgu.ac.il>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-02-26 18:18:04 -06:00
Paul Romano
3b5ac08bfb
Skip DAGMC lost particles test (#3836) 2026-02-26 11:26:39 -06:00
Paul Romano
17d4164242
Update copyright to 2026 (#3834) 2026-02-26 08:14:28 +00:00
GuySten
322b741fde
Support Mixture distributions in combine_distributions (#3784)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-02-26 07:30:08 +00:00
Jonathan Shimwell
6050c789ca
making use of endf.get_evaluations (#3819)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-02-26 03:14:44 +00:00
GuySten
3ba8a9f078
Correctly score pulse height tally when no cell filter is present (#3821)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-02-26 02:44:17 +00:00
Jonathan Shimwell
8081815b99
Add RegularMesh.get_indices_at_coords method (#3824)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-02-26 02:19:02 +00:00
John Tramm
54c8e3d6eb
Speedup CI and Improve Reproducibility Across Compilers (#3823)
Co-authored-by: John Tramm <jtramm@gmail.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-02-25 17:12:18 -06:00
GuySten
2a38dc11ec
Do not fail CI when coveralls.io is not available. (#3835) 2026-02-25 15:04:00 -06:00
GuySten
c0427dd40a
Resolve conflict with weight windows and global russian roulette (#3751)
Co-authored-by: Patrick Shriwise <pshriwise@gmail.com>
2026-02-25 14:01:33 -06:00
Patrick Shriwise
5a85bd92f2
C++ formatting suggestions on PRs (#3829) 2026-02-25 11:08:04 -06:00
Jonathan Shimwell
3ff6b59a49
Allow Mesh.from_domain to use bounding boxes directly (#3828) 2026-02-24 23:44:30 -06:00
Paul Romano
e130701f10
Fix MeshFilter.get_pandas_dataframe to handle all mesh types (#3817) 2026-02-24 07:35:23 +00:00
Vitaly Mogulian
8c24c1c064
Modify the plotter ray tracing for its utilization in estimators (#3816)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-02-24 06:46:21 +00:00
GuySten
83a30f6860
Support arbitrary symmetry axis for CylindricalIndependent class (#3474)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-02-21 20:00:36 +00:00
Paul Romano
139907c955
Implement tally filter for filtering by reaction (#3809) 2026-02-21 10:17:12 -06:00
Jonathan Shimwell
153281a490
Remove unused class Tabulated2D (#3818) 2026-02-21 15:00:22 +00:00
John Tramm
53ce1910f9
Fix S2 Random Ray Casting Issue (#3825) 2026-02-19 18:25:31 +00:00
Kevin Sawatzky
efefdb17b1
Add more operator overloads in the new Tensor class (#3822) 2026-02-19 11:03:19 -06:00
Kevin Sawatzky
417343c920
Implement S2 directional sampling in the random ray solver (#3811) 2026-02-19 14:25:19 +02:00
GuySten
f007c85a50
Check for positive radii (#3813) 2026-02-19 08:36:12 +00:00
Jonathan Shimwell
6d6b051507
avoid need to set particles and batches for dagmc models when calling convert_to_multigroup (#3801)
Co-authored-by: Jon Shimwell <jon@proximafusion.com>
Co-authored-by: Patrick Shriwise <pshriwise@gmail.com>
Co-authored-by: GuySten <62616591+GuySten@users.noreply.github.com>
2026-02-18 11:18:05 -06:00
GuySten
d4dc089618
Remove redundant check (#3812) 2026-02-18 09:09:39 -06:00
John Tramm
977ade79a1
Replace xtensor with internal Tensor/View classes (#3805)
Co-authored-by: John Tramm <jtramm@gmail.com>
2026-02-17 09:50:38 -06:00
Kevin Sawatzky
c6ef84d1d5
Set upper and lower interpolation bounds for MGXS data. (#3803) 2026-02-15 23:59:08 +02:00
Paul Romano
a35927aad3
Extend ParticleProductionFilter to support multiple particle types (#3780) 2026-02-13 22:18:29 -06:00
GuySten
7fc5b94877
Store atomic mass in ParticleType. (#3765)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-02-14 03:14:03 +00:00
Kevin Sawatzky
19c0aafdc6
Fix None values appearing in cross section data generated with Model.autoconvert (#3802) 2026-02-13 18:52:10 +02:00
Patrick Shriwise
bcb9395207
SolidRayTracePlot CAPI (#3789)
Co-authored-by: GuySten <62616591+GuySten@users.noreply.github.com>
2026-02-13 07:54:27 +02:00
GuySten
b145fdd999
Improve radial crossing checks in SphericalMesh and CylindricalMesh (#3792)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-02-13 05:10:20 +00:00
Jonathan Shimwell
4e5deed0cc
Using ``_LIBRARY` and `_SUBLIBRARY`` from endf package (#3804) 2026-02-13 03:25:49 +00:00
Paul Romano
8198e6021d
Add truncated normal distribution support (#3761) 2026-02-12 18:25:56 +02:00
Patrick Shriwise
a3426cf833
Fix weight windows regression test (#3798) 2026-02-12 06:30:31 -06:00
Jonathan Shimwell
8d0fe6c71d
making use of sum_rules in endf package (#3799) 2026-02-12 10:11:28 +00:00
Jonathan Shimwell
26b13083f3
Use gnds_name and zam from endf package (#3796) 2026-02-12 05:58:00 +00:00
GuySten
96383fcb2b
More interpolation types in Tabular. (#3413)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-02-11 21:05:07 +00:00
azim-givron
360ec24b41
Implement vector fitting to replace external vectfit package (#3493)
Co-authored-by: azim_givron <a.givron@naarea.fr>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
Co-authored-by: GuySten <guyste@post.bgu.ac.il>
Co-authored-by: GuySten <62616591+GuySten@users.noreply.github.com>
2026-02-11 10:00:18 -06:00
Matthew Feickert
44da7022b8
FIX: Remove setuptools from run dependencies (#3794) 2026-02-11 09:21:13 -06:00
Jonathan Shimwell
3f20a5e228
Use several data variables from endf package (#3787) 2026-02-10 06:41:04 -06:00
Jonathan Shimwell
8053111f2d
making use of endf-python package more (#3786)
Co-authored-by: GuySten <guyste@post.bgu.ac.il>
2026-02-10 02:08:25 +00:00
Kevin Sawatzky
4f4930b633
Temperature feedback support in the random ray solver. (#3737) 2026-02-09 16:54:59 -06:00
Paul Romano
d0346e94ac
Install parallel h5py with no build isolation (#3782) 2026-02-08 22:22:39 +00:00
Patrick Shriwise
6efc9db7b3
Modifications to C++ plots for interactive raytrace plots (#3776) 2026-02-08 12:11:19 -06:00
GuySten
04bee9c49f
Check that Surface IDs are at least 1 (#3772)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-02-06 18:44:16 +00:00
Lewis Gross
a632429267
Move distrib (mat, temp, dens) from XML attribute to subelement for better compatibility with very large instance lists (#3774) 2026-02-06 19:32:32 +02:00
Kevin Sawatzky
14acc762bc
C-API bindings for key random ray functions (#3749) 2026-02-06 10:42:32 -06:00
Jonathan Shimwell
8a62a97115
openmc.Tally creation from constructor (#3777) 2026-02-06 10:23:11 -06:00
Jonathan Shimwell
6f625f3dea
Precompute offsets in random ray source update (#3775) 2026-02-06 09:25:14 -06:00
Gavin Ridley
f2c936cf5b
Implement filter for secondary particle production binned by energy (#3453)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-02-05 18:00:03 -06:00
Jonathan Shimwell
1039b5d9ff
Parallelize transpose of scattering matrix for random ray adjoints (#3768) 2026-02-05 10:43:16 -06:00
Paul Romano
3b619d6904
Fix use of length multiplier in several LibMesh methods (#3773) 2026-02-04 22:29:30 -06:00
David Andrs
a22238e069
Fixing compiler warning about VLA (Clang extension) (#3769) 2026-02-04 14:50:38 -06:00
Paul Romano
b41e22f68b
Refactor ParticleType to use PDG Monte Carlo numbering scheme (#3756)
Co-authored-by: GuySten <62616591+GuySten@users.noreply.github.com>
Co-authored-by: Amanda Lund <alund1187@gmail.com>
2026-02-03 07:23:24 +00:00
Ethan Peterson
fc0d9eec65
Ignore all source build directories that match build* pattern (#3762) 2026-02-02 09:55:45 -06:00
David Andrs
6041ee6ae3
SpatialBox can be constructed via ctor with parameters (#3760) 2026-01-31 17:02:39 -06:00
GuySten
7b4617affb
Fix for plotting model with multi-group cross sections (#3748)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-01-30 06:10:16 +00:00
Paul Romano
f7a734189a
Optionally compute bounding boxes in Mesh.material_volumes (#3731) 2026-01-29 09:20:48 +02:00
GuySten
008d584607
Warn users when setting undefined attributes in ``openmc.Settings`` (#3746)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-01-28 08:02:02 +00:00
Jonathan Shimwell
db426b66ca
Materials name persist when running depletion simulation (#3738)
Co-authored-by: GuySten <guyste@post.bgu.ac.il>
Co-authored-by: GuySten <62616591+GuySten@users.noreply.github.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-01-27 06:06:36 +00:00
Paul Romano
5c502ddb3e
Do not add radioactive Ta180 when calling add_element('Ta') (#3750) 2026-01-26 19:09:58 +02:00
Kevin Sawatzky
3e2f1f521a
Enable fission heating tallies in the random ray solver (#3714) 2026-01-23 10:23:05 -06:00
Olek
73a98b2cc6
Add random_ray_pincell() example model (#3735)
Co-authored-by: John Tramm <john.tramm@gmail.com>
2026-01-23 10:20:25 -06:00
Olek
049a852e52
Random Ray main function and autosetup refactoring (#3733) 2026-01-22 15:21:47 -06:00
GuySten
6b43a298f4
Add n_elements to the MeshBase protocol and deprecate num_mesh_cells (#3745) 2026-01-22 15:04:30 +00:00
GuySten
c5df2bf621
Fix for pandas version 3 (#3743) 2026-01-21 21:57:40 -06:00
GuySten
2691ff8a0f
Fix type hinting and simplify implementation of combine_distributions (#3445)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-01-21 14:33:30 +00:00
Kevin Sawatzky
5847b0de23
Block restriction of libMesh unstructured mesh tallies (#3694) 2026-01-17 04:01:37 +00:00
Paul Romano
51ea89ccc8
Implement depth-awareness when enforcing precedence between union/intersection operators (#3730)
Co-authored-by: GuySten <guyste@post.bgu.ac.il>
2026-01-15 22:23:35 -06:00
GuySten
179048b801
Skip tests on documentation-only changes (#3727)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-01-14 23:24:07 -06:00
Paul Romano
7861adf53b
Add git branching information to AGENTS.md (#3726) 2026-01-14 13:29:24 -06:00
Kevin Sawatzky
5bce5adabc
Support cell densities in the random ray solver (#3720) 2026-01-14 20:02:17 +02:00
GuySten
7106958e00
Simplify IFP message passing (#3719)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-01-13 23:25:33 +00:00
GuySten
65e19c1d53
Fix settings io_format documentation. (#3718)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-01-13 21:31:01 +00:00
Jonathan Shimwell
84a413b130
Speed up reaction rate lookup for FluxCollapseHelper (#3724) 2026-01-13 15:34:07 -05:00
Jack Fletcher
0486e433d2
Source biasing capabilities (#3460)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-01-12 09:51:12 -06:00
Perry
37e2feb34b
Flux Energy Group Conversion using lethargy-weighted redistribution (#3705)
Co-authored-by: GuySten <62616591+GuySten@users.noreply.github.com>
2026-01-10 22:04:47 +02:00
Paul Romano
8c8867ea1c
Add --merge-mode-functions=separate to gcovr call in CI (#3716) 2026-01-09 20:05:51 +00:00
GuySten
551bf0730b
Simplify translational periodic boundary conditions (#3697) 2026-01-09 07:56:40 -06:00
Jonathan Shimwell
dfc80c7069
fixing temperatures setting for mgxs (#3712) 2026-01-07 10:54:57 +00:00
Paul Romano
830f075b5c
Update documentation describing HexLattice orientation (#3709) 2026-01-06 22:59:58 +00:00
Jonathan Shimwell
7dceb1d80a
closing mgxs h5py file with context manager (#3707)
Co-authored-by: GuySten <62616591+GuySten@users.noreply.github.com>
2026-01-06 22:59:38 +00:00
Jonathan Shimwell
10f2b7534c
Fixing group names in MGXS HDF5 file (#3708) 2026-01-06 20:18:23 +00:00
GuySten
c7d7fa4613
Fix a bug in rotational periodic boundary conditions (#3692)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-01-06 13:29:40 +00:00
GuySten
818fd11b18
Simplify rectangular lattice crossing and correctly handle corner checks (#3703)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2026-01-06 09:29:46 +00:00
Jonathan Shimwell
60ddafa9b3
Open dagmc model file within a context manager (#3706) 2026-01-05 22:57:05 +02:00
Paul Romano
9c91bddf04
Migrate to SciPy sparse arrays (#3613) 2026-01-02 13:43:25 +02:00
Paul Romano
932f36f411
Add recognized thermal scattering names for JEFF 4.0 and JENDL 5 (#3693) 2026-01-02 12:31:46 +02:00
GuySten
f08326a9ac
Cache cross sections according to the hash of download-xs.sh script (#3701) 2026-01-01 13:30:09 +02:00
Paul Romano
92d7fdb199
Use min/max position members in C++ BoundingBox class (#3699) 2025-12-30 21:31:53 -06:00
GuySten
3f06a42abb
Refactor get_energy_index to prevent repetition (#3686) 2025-12-23 14:18:59 -06:00
Zoe Prieto
a2fd6cc57e
Support rotation in MeshFilter (#3176)
Co-authored-by: Jonathan Shimwell <drshimwell@gmail.com>
Co-authored-by: Patrick Shriwise <pshriwise@gmail.com>
2025-12-19 22:56:13 -06:00
GuySten
a230b86128
Fix mcpl dependency in test (#3691) 2025-12-18 15:56:43 +00:00
Jonathan Shimwell
e0eb91b955
using id_map in model.plot for more efficient plotting (#3678) 2025-12-17 22:44:53 +02:00
Patrick Shriwise
d118356638
Use MeshBase method to check replicated. Add header for replicated mesh (#3689) 2025-12-17 06:10:07 +00:00
Kevin Sawatzky
bbfa18d72c
Add a command-line argument for output verbosity (#3680)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-12-12 09:29:43 +00:00
GuySten
1b5033dab4
IFP creates fatal error in all run modes except eigenvalue. (#3681) 2025-12-12 00:21:46 -06:00
GuySten
5c4121efd2
Fix hdf5 source_bank struct size. (#3676) 2025-12-11 22:01:10 -06:00
pranav
a62e754bbb
Add user documentation for DAGMCUniverse synchronization (#3674)
Co-authored-by: Patrick Shriwise <pshriwise@gmail.com>
2025-12-10 21:54:28 -06:00
John Tramm
d09fbc61b5
Copilot Bot File (#3651)
Co-authored-by: Copilot <175728472+Copilot@users.noreply.github.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
Co-authored-by: Patrick Shriwise <pshriwise@gmail.com>
2025-12-10 09:26:26 -06:00
Lewis Gross
bc1348579f
Generalize RotationalPeriodicBC for X-, Y-, or Z-axis (#3591)
Co-authored-by: GuySten <62616591+GuySten@users.noreply.github.com>
2025-12-10 12:16:04 +02:00
Jonathan Shimwell
a9dc84f75a
Allowing material making from class constructor (#3649)
Co-authored-by: Jon Shimwell <jon@proximafusion.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-12-08 19:43:30 +00:00
Jonathan Shimwell
8e06ed8998
Allowing model.id_map to return overlap ID values (#3669)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-12-08 15:54:37 +00:00
GuySten
9b40ea008e
Read IFP settings only in source/eigenvalue run mode (#3673) 2025-12-08 05:39:48 -06:00
Paul Romano
f70febb05f
Update CITATION.cff file (#3671) 2025-12-06 21:54:30 +00:00
Boris Polania
9b675adda5
Introduce SlicePlot and VoxelPlot to replace the Plot class (#3528)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-12-05 20:17:09 +00:00
Jonathan Shimwell
f28139250a
Fixed plotting issue by scaling source locations with axis units (#3668) 2025-12-05 11:02:26 -06:00
Paul Romano
db8d462738
Allow DistribcellFilter to work with apply_tally_results=True (#3667) 2025-12-04 06:53:04 -06:00
John Tramm
ad5a876bee
Improved automatic MGXS generation for random ray (#3658)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-12-03 07:48:38 +00:00
John Tramm
10706510bf
Random Ray Eigenvalue Flux Normalization Change (#3595)
Co-authored-by: Copilot <175728472+Copilot@users.noreply.github.com>
2025-12-02 22:00:32 -06:00
Paul Romano
9e9ab84833
Update C++/CMake policy based on Ubuntu 22.04 (#3666) 2025-12-02 16:11:56 +00:00
GuySten
ef22558f4a
fix a bug in borated_water temperature assignment (#3662) 2025-11-29 16:28:18 +01:00
Paul Romano
7ab92ec142
Fix typo in description of distance_inactive for random ray setting (#3663) 2025-11-28 15:39:08 +00:00
Jonathan Shimwell
dcb7443711
added test to check dagmc name is in xml (#3657) 2025-11-27 10:03:38 -06:00
Paul Romano
27e38e8946
Add release notes for 0.15.3 (#3644) 2025-11-22 23:06:17 +01:00
Paul Romano
d217efa007
Add two MPI barriers in R2S workflow (#3646) 2025-11-20 12:10:04 -06:00
Paul Romano
f544d02e49
Don't write reaction rates in depletion results by default, remove per-stage data for multistage integrators (#3609) 2025-11-19 12:26:57 -05:00
Paul Romano
028f440448
Support MPI parallelism in R2SManager (#3632) 2025-11-19 11:19:27 -06:00
Paul Romano
5c63e0df21
Fix a few warnings, rename add_to_tallies_file (#3639) 2025-11-18 17:57:12 -06:00
Patrick Shriwise
7815d3a680
Fix typo in DAGMC lost particle test (#3634) 2025-11-14 05:27:17 +00:00
Paul Romano
8d618716b5
Avoid multiprocessing Pool when running depletion tests with MPI (#3633) 2025-11-13 17:14:39 -06:00
Michel Saliba
cd5cd35ad9
Addition of a collision tracking feature (#3417)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-11-13 20:35:33 +00:00
Lorenzo Chierici
50bb0df191
depletion-thermochemistry: Redox control transfer rates (#2783)
Co-authored-by: Gavin Ridley <gavin.keith.ridley@gmail.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-11-12 16:45:48 -06:00
April Novak
4e24c2d933
Update documentation for particle tracks (#3627)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-11-12 21:59:45 +00:00
Gregoire Biot
2d77544b0c
Adding variance of variance and normality tests for tally statistics (#3454)
Co-authored-by: Ethan Peterson <eepeterson3@gmail.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-11-12 11:41:37 -05:00
Marco De Pietri
e5348d3f62
Avoid divide-by-zero in from_multigroup_flux when flux is zero (#3624)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-11-12 10:35:07 +00:00
Patrick Shriwise
5c2bfe771e
Write particle states as separate lines in track VTK files. (#3628) 2025-11-12 00:29:19 -06:00
Patrick Shriwise
8cd3911cbe
Reset DAGMC history when reviving from source. (#3601)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-11-12 06:01:18 +00:00
Perry
c0f302db68
Add energy group structure: SCALE-999 (#3564) 2025-11-07 10:58:40 -06:00
Jon Shimwell
e5c7d0ca88
Adding vtkhdf option to write vtk data (#3252)
Co-authored-by: shimwell <mail@jshimwell.com>
Co-authored-by: Jonathan Shimwell <drshimwell@gmail.com>
Co-authored-by: rherrero-pf <156206440+rherrero-pf@users.noreply.github.com>
Co-authored-by: Patrick Shriwise <pshriwise@gmail.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-11-05 16:03:20 +00:00
Paul Romano
bd76fc0566
Fix bug in normalization of tally results with no_reduce (#3619) 2025-11-03 11:11:57 -06:00
Perry
2d8e006c3d
Enable nuclide filters with get_decay_photon_energy (#3614)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-11-03 11:10:30 -06:00
GuySten
fd964bc9b0
Enable specifying reference direction for azimuthal angle in PolarAzimuthal distribution (#3582)
Co-authored-by: shimwell <mail@jshimwell.com>
2025-11-03 09:42:59 +02:00
Paul Romano
5fc289b99d
Automate workflow for mesh- or cell-based R2S calculations (#3508)
Co-authored-by: Ethan Peterson <eepeterson3@gmail.com>
Co-authored-by: Jonathan Shimwell <drshimwell@gmail.com>
2025-11-01 00:15:25 +00:00
Paul Romano
4c41766611
Criticality search method on the Model class (#3569) 2025-10-28 11:36:03 -05:00
Makarand More
a74c1424a8
Update check_type calls to accept both str and os.PathLike objects. (#3618)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-10-28 14:50:11 +00:00
Paul Romano
f10d7d9f67
Speed up apply_time_correction by reducing file I/O and deepcopies (#3617) 2025-10-28 09:23:16 +01:00
John Tramm
230db28d39
FW-CADIS Disregard Max Realizations Setting (#3616) 2025-10-28 09:22:37 +01:00
John Tramm
70b5254662
Random Ray Geometry Debug Mode Fix (#3615) 2025-10-27 09:30:54 +01:00
GuySten
c31032cf25
load mesh objects from weight_windows.h5 file (#3598)
Co-authored-by: Patrick Shriwise <pshriwise@gmail.com>
2025-10-21 23:03:27 +00:00
Jonathan Shimwell
3ac5d6f8f5
Allow Path objects in MGXSLibrary.export_to_hdf5 (#3608)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-10-20 16:45:14 +00:00
Paul Romano
055ea15a2d
Clip mixture distributions based on mean times integral (#3603) 2025-10-17 18:09:37 -05:00
GuySten
b94b496113
Ability to source electron/positrons directly (#3404)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-10-15 23:51:59 +00:00
jiankai-yu
e9077b1372
Allow V0 in atomic_mass function (for ENDF/B-VII.0 data) (#3607) 2025-10-14 20:21:11 +00:00
Paul Romano
58c7fbeac6
Re-run flaky tests when needed (#3604) 2025-10-14 07:47:26 -05:00
Paul Romano
3dfa34d2c6
Switch to using coveralls github action for reporting (#3594) 2025-10-07 05:14:37 +03:00
Paul Romano
2c15480cc9
Add user setting for free gas threshold (#3593) 2025-10-06 15:45:26 +03:00
Jonathan Shimwell
50071aa3bd
Speed up time correction factors (#3592)
Co-authored-by: Jon Shimwell <jon@proximafusion.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-10-03 15:09:57 +00:00
Thomas Kittelmann
8a62e7e323
Fix caching issue when using NCrystal materials (#3538)
Co-authored-by: Jose Ignacio Marquez Damian <22483345+marquezj@users.noreply.github.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-10-02 23:27:36 +00:00
Copilot
7806703c26
Fix random ray source region mesh export when using model.export_to_xml() (#3579)
Co-authored-by: copilot-swe-agent[bot] <198982749+Copilot@users.noreply.github.com>
Co-authored-by: jtramm <1009059+jtramm@users.noreply.github.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-10-02 22:52:39 +00:00
Perry
91a19cf220
Ensure weight_windows_file information is read from XML (#3587)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-10-02 21:50:42 +00:00
Patrick Shriwise
1dacf4fd2b
Add missing documentation on <source> in depletion chain file format (#3590)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
Co-authored-by: April Novak <novak@berkeley.edu>
2025-10-02 16:48:02 +00:00
John Tramm
3ac64d9a01
Random Ray Base Source Region Refactor (#3576) 2025-10-02 11:02:43 -05:00
Jonathan Shimwell
feefcc6713
Adding tally filter type option to statepoint get_tally (#3584)
Co-authored-by: Jon Shimwell <jon@proximafusion.com>
Co-authored-by: GuySten <62616591+GuySten@users.noreply.github.com>
2025-09-30 22:09:15 +00:00
Perry
4011b7a551
Optional separation of mesh-material-volume calc from get_homogenized_materials (#3581)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-09-26 16:46:23 +00:00
Alex Nellis
781dbf9c12
Multi-group capability for kinetics parameter calculations with Iterated Fission Probability (#3425)
Co-authored-by: GuySten <guyste@post.bgu.ac.il>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-09-26 16:27:05 +00:00
Joffrey Dorville
767db7e6a0
Fix IFP implementation (#3580) 2025-09-25 14:58:29 -05:00
GuySten
66e7d8634c
Remove several TODOs related to C++17 support (#3574)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-09-24 09:02:19 +00:00
Kevin Sawatzky
ed433fe1cd
Fix performance regression in libMesh unstructured mesh tallies (#3577) 2025-09-23 11:31:14 -05:00
Paul Romano
8f36ff2b3a
Update find_package calls in OpenMCConfig.cmake (#3572) 2025-09-23 10:06:29 -05:00
Patrick Shriwise
ca63da91b9
Ensure n_dimension_ attribute is set for unstructured meshes. (#3575) 2025-09-19 20:00:51 +00:00
Ilham Variansyah
ecb0a3361f
Combing for fission site sampling, and delayed neutron emission time (#2992)
Co-authored-by: Gavin Ridley <gavin.keith.ridley@gmail.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-09-19 08:10:08 +00:00
Paul Romano
007ac8148b
Allow newer Sphinx version and fix docbuild warnings (#3571) 2025-09-19 07:27:41 +03:00
Kevin Sawatzky
607f6babe5
Add distributed cell densities (#3546)
Co-authored-by: Patrick Shriwise <pshriwise@gmail.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-09-19 04:11:06 +00:00
GuySten
afd9d06074
Fixed a bug when combining TimeFilter, MeshFilter, and tracklength estimator (#3525)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-09-12 20:23:17 +00:00
Jack Fletcher
c7175289eb
PowerLaw raises an error if sampling interval contains negative values (#3542) 2025-09-11 15:57:02 +03:00
Robert Carlsen
ca4295748d
depletion: fix performance of chain matrix construction (#3567)
Co-authored-by: GuySten <62616591+GuySten@users.noreply.github.com>
2025-09-11 02:13:28 +00:00
Patrick Shriwise
3665090513
Do not apply boundary conditions when initialized in volume calculation mode (#3562) 2025-09-05 11:34:49 +00:00
Paul Romano
5918564727
Bump up tolerance for flaky activation test (#3560) 2025-09-03 16:35:11 +00:00
GuySten
eaed400987
Fixed a bug in plotting cross sections with S(a,b) data (#3558) 2025-09-02 22:52:27 -05:00
GuySten
00edc77691
Change test order to run unit tests first. (#3533)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-08-30 03:39:46 +00:00
Jonathan Shimwell
ec15803d41
adding ecco 33 (#3556) 2025-08-30 04:39:45 +03:00
GuySten
5529731e2f
Refactor endf_data to be a fixture (#3539) 2025-08-29 07:06:33 -05:00
GuySten
2a278c93a6
Revert "fix broken CI" (#3554) 2025-08-27 23:18:06 +00:00
GuySten
b14eff4760
fix broken CI (#3551) 2025-08-27 19:28:11 +00:00
GuySten
d1df80a210
Leverage particle.move_distance in event advance (#3544) 2025-08-22 09:58:39 -05:00
GuySten
5e3249f006
fix tests that accidentaly got broken (#3543) 2025-08-21 21:13:50 +00:00
Jonathan Shimwell
e878aeb82f
not printing nuclides with 0 percent to terminal (option 2 ) (#3448) 2025-08-21 11:14:21 +02:00
GuySten
68e894c4b0
Fix a bug in time cutoff behavior (#3526) 2025-08-18 09:40:54 -05:00
Rémi Delaporte-Mathurin
c5a7173864
Avoid duplicate materials written to XML (#3536)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-08-18 14:34:12 +00:00
GuySten
75b5813012
Use cached property for openmc.data.Decay.sources (#3535)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-08-18 13:42:38 +00:00
Jonathan Shimwell
14d51e0eba
more helpful error message for dose_coefficients (#3534) 2025-08-14 21:26:27 +03:00
Jonathan Shimwell
f8fa751da0
Adding 616 group structure (#3531) 2025-08-13 16:41:39 +03:00
GuySten
a34365396e
Remove unused special accessors for tallies (#3527) 2025-08-11 10:51:45 -05:00
GuySten
a11021cd07
Consistent XML parsing using functions from _xml module (#3517)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-08-08 17:47:55 +00:00
Boris Polania
e36c0aef2f
Add stat:sum field to MCPL files for proper weight normalization (#3522)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-08-08 14:09:24 +00:00
GuySten
4500f07b44
Remove reorder_attributes from openmc._xml (#3519) 2025-08-08 16:59:22 +07:00
GuySten
4fabed542d
fixed a bug in MeshMaterialFilter.from_volumes (#3520)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-08-08 00:53:33 +00:00
GuySten
a64cc96ed5
Fixed a bug in distribcell offsets logic (#3424) 2025-07-30 12:10:34 -05:00
Jonathan Shimwell
6f5e1347d4
Add test for FW-CADIS based WW generation on a DAGMC model (#3504)
Co-authored-by: Jon Shimwell <jon@proximafusion.com>
Co-authored-by: Patrick Shriwise <pshriwise@gmail.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-07-29 11:17:51 +00:00
John Tramm
4cce6ee6c0
Fix for Weight Window Scaling Bug (#3511)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-07-29 10:15:40 +00:00
Rémi Delaporte-Mathurin
836bc487cf
Fix: materials, plots, and tallies cannot be passed as lists (#3513)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-07-29 09:34:03 +00:00
Paul Romano
6b672f772f
Allow already-initialized openmc.lib in TemporarySession (#3505) 2025-07-26 16:42:33 -05:00
Patrick Shriwise
9d9dcc26c5
Update DAGMC and libMesh precompiler definitions (#3510) 2025-07-22 11:10:08 +07:00
Jonathan Shimwell
a649d7bc69
Avoid adding ParentNuclideFilter twice when calling prepare_tallies (#3506)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-07-18 16:23:02 +00:00
Jonathan Shimwell
8be65513b7
Adding material depletion function (#3420)
Co-authored-by: Jon Shimwell <jon@proximafusion.com>
Co-authored-by: Micah Gale <mgale@fastmail.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-07-18 14:37:57 +00:00
Joffrey Dorville
659e43af7d
Enabling MCPL source files to be read when using surf_source_read (#3472)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-07-18 08:47:08 +00:00
Patrick Shriwise
637e04a9ba
Boundary info accessors (#3496)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-07-18 07:51:30 +00:00
Jonathan Shimwell
4483583ddd
automatically finding appropriate dimension when making regular mesh from domain (#3468) 2025-07-18 13:46:13 +07:00
Patrick Shriwise
bca818ced6
Add accessor methods for LocalCoord (#3494)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-07-17 03:29:41 +00:00
Ahnaf Tahmid Chowdhury
5318ea6e2b
Make MCPL a Runtime Optional Dependency (#3429)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-07-17 02:46:39 +00:00
Perry
24f78e6e92
Use auto-chunking for StepResult HDF5 writing (#3498) 2025-07-17 08:40:02 +08:00
Patrick Shriwise
6372c29cfa
Provide a way to get ID maps from plot parameters on the Model class (#3481)
Co-authored-by: Jonathan Shimwell <drshimwell@gmail.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-07-16 08:31:49 -05:00
Shikhar Kumar
58ee8d825d
Update OSX install instructions to point to x64 platform (#3501) 2025-07-15 15:53:52 -05:00
Paul Romano
d700d395de
Update conda install instructions for macOS Apple silicon (#3488) 2025-07-03 22:59:40 +00:00
April Novak
dd8d621f0b
Only show warning if in restart mode. Refs #3477 (#3478) 2025-07-03 10:10:12 -05:00
Nathan Glaser
b6c6ac078b
Add flag to CMakeLists to use submodules instead of searching (#3480)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-07-03 14:49:25 +00:00
Micah Gale
efcf8f649e
Added citation metadata file (#3409) 2025-07-03 10:32:43 +02:00
GuySten
6636b7e32b
fix zam parsing (#3484) 2025-07-02 22:52:39 -05:00
Paul Romano
eb74d497d2
Introduce openmc.lib.TemporarySession context manager (#3475) 2025-07-01 12:43:45 -05:00
Paul Romano
ecfb666db7
Allow spatial constraints on element sources within MeshSource (#3431) 2025-07-01 09:03:28 -05:00
Paul Romano
dab8af5672
Support flux collapse method in get_microxs_and_flux (#3466)
Co-authored-by: Jonathan Shimwell <drshimwell@gmail.com>
2025-07-01 12:43:28 +02:00
John Tramm
b939f9003b
Stabilize Adjoint Source (#3476) 2025-06-30 10:33:22 +02:00
Ahnaf Tahmid Chowdhury
25d64c9b26
Refactor and Harden Configuration Management (#3461)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-06-27 00:49:55 +00:00
John Tramm
c116288ea3
Updated Docs to Not Give Specific Python Version Requirement (#3473) 2025-06-26 23:50:26 +00:00
Jonathan Shimwell
5c10214465
added openmc.Material.mean_free_path function (#3469) 2025-06-25 20:29:45 -05:00
Paul Romano
01fa8056d1
Introduce WeightWindowsList class that enables export to HDF5 (#3456) 2025-06-25 13:44:53 -05:00
John Tramm
a6db05ac8b
Optimize Mapping of Random Ray Source Regions to Tallies (#3465) 2025-06-25 08:47:23 -05:00
John Tramm
15dfe7e8b9
Parallelization of Weight Window Update (#3467) 2025-06-25 08:46:40 -05:00
John Tramm
2a0299aec7
Limit Random Ray Weight Window Generation to Final Batch (#3464) 2025-06-24 15:20:26 -05:00
Paul Romano
3a8894c3f8
Fix Dockerfile DAGMC build (#3463) 2025-06-24 11:29:16 +02:00
John Tramm
7c6aaf7204
Fix Weight Window Infinite Loop Bug (#3457)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-06-23 22:20:36 +00:00
John Tramm
eaef13b9bc
Weight Window Birth Scaling (#3459)
Co-authored-by: Copilot <175728472+Copilot@users.noreply.github.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-06-23 20:53:27 +00:00
Jonathan Shimwell
3d16d4b100
Adding checks to geometry.plot to avoid material name overlaps (#3458)
Co-authored-by: Patrick Shriwise <pshriwise@gmail.com>
2025-06-19 20:43:45 +00:00
Jonathan Shimwell
3e32aed2da
Fixing crash when calling Geometry.plot when DAGMCUniverse in geometry (#3455)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-06-18 18:34:07 +00:00
GuySten
1c5aa6559b
fixing expansion of elemental Ta bug (#3443)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-06-18 15:10:03 +00:00
John Tramm
f31130d367
Prevent Adjoint Sources from Trending towards Infinity (#3449) 2025-06-18 06:34:56 -05:00
Jonathan Shimwell
7a1cafa6c1
adding plot function to DAGMCUnvierse (#3451)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-06-17 22:36:35 +00:00
Jan Malec
23eab2c89b
Allow specifying number of equiprobable angles for thermal scattering data generation (#3346)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-06-14 06:39:31 +00:00
Paul Romano
b11eb02655
Change Dockerfile from debian:bookworm-slim to ubuntu:24.04 (#3442) 2025-06-13 20:38:16 +00:00
John Tramm
aeb1052c19
Fix Resetting of Auto IDs When Generating MGXS (#3437) 2025-06-13 00:54:35 +00:00
Jonathan Shimwell
f81962c960
Allowing chain_file to be chain object to save reloading time (#3436)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-06-12 21:02:35 +00:00
April Novak
6c9c69628c
update units for flux (#3441) 2025-06-12 16:49:59 +00:00
GuySten
e678b1a057
Fix raytrace infinite loop. (#3423)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-06-11 22:54:04 +00:00
John Tramm
2eeba89992
Apply Max Number of Events Check to Random Rays (#3438)
Co-authored-by: Jonathan Shimwell <drshimwell@gmail.com>
2025-06-11 12:41:38 -05:00
Paul Romano
f571be87c5
Add user setting for source rejection fraction (#3433) 2025-06-10 22:51:51 -05:00
Patrick Shriwise
f796fa04e0
Adding fix and tests for spherical mesh as spatial distribution (#3428)
Co-authored-by: Paul Wilson <paul.wilson@wisc.edu>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-06-10 10:01:28 -05:00
John Tramm
56b44aa4e8
Random Ray Missed Cell Policy Change for Adjoint Mode (#3434) 2025-06-10 09:13:08 -05:00
Paul Romano
7fda3eb846
Implement a new MeshMaterialFilter (#3406)
Co-authored-by: Jonathan Shimwell <drshimwell@gmail.com>
Co-authored-by: Patrick Shriwise <pshriwise@gmail.com>
2025-06-06 16:30:50 -05:00
John Tramm
67aa0def9d
Random Ray External Source Plotting Fix (#3430) 2025-06-06 14:51:39 -05:00
Paul Romano
4943fa3630
Avoid negative heating values during pair production and bremsstrahlung (#3426)
Co-authored-by: GuySten <guyste@post.bgu.ac.il>
2025-06-05 10:45:49 -05:00
GuySten
dadc4fe418
Fix no serialization of periodic_surface_id bug (#3421)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-06-05 00:07:59 +00:00
Lewis Gross
e14bb884eb
Update _get_start_data to always grab the beginning of timestep time (#3414)
Co-authored-by: Paul Wilson <paul.wilson@wisc.edu>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-06-04 23:40:55 +00:00
GuySten
ace73ab5de
Fixed a bug in charged particle energy deposition. (#3416)
Co-authored-by: Jonathan Shimwell <drshimwell@gmail.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-06-03 18:02:20 +00:00
GuySten
cb95c784b7
Fix bug where the same mesh is written multiple times to settings.xml (#3418) 2025-05-27 11:04:16 -05:00
Alberto P
a7d1ceba3f
small typo - spelling of Debian (#3411) 2025-05-18 20:28:00 +03:00
Jonathan Shimwell
757617be50
added test for dagmc geometry plot (#3375)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-05-16 13:55:41 +00:00
Lorenzo Chierici
7382b5d1c8
External transfer rates source term (#3088)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-05-12 15:48:21 -05:00
John Tramm
f615441f06
Random Ray Misc Memory Error Fixes (#3405)
Co-authored-by: Hunter Belanger <hunter.belanger@gmail.com>
2025-05-09 22:10:25 -05:00
Jonathan Shimwell
ba834be5c2
added type hints to model file (#3399)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-05-08 06:10:33 +00:00
Patrick Shriwise
c1c5c0b93e
Apply resolve paths to path values in config (#3400) 2025-05-08 00:51:40 +00:00
GuySten
f9dca9a458
Fixing an incorrect computation of CDF of bremsstrahlung photons (#3396)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-05-06 00:04:47 +00:00
Paul Romano
e4f55a57b6
Fix weight modification for uniform source sampling (#3395)
Co-authored-by: Patrick Shriwise <pshriwise@gmail.com>
2025-05-05 20:59:11 +00:00
Gregoire Biot
dc619eac17
Filter weight implementation (#3345)
Co-authored-by: Grego01-biot <grego01@pc-neutronic-06.psfc.mit.edu>
Co-authored-by: Patrick Shriwise <pshriwise@gmail.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-05-05 15:33:12 -05:00
Patrick Shriwise
9942269a91
Updates to VTK data checks (#3371)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-05-05 18:55:14 +00:00
Amanda Lund
57dc71f530
Map Compton subshell data to atomic relaxation data (#3392)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-05-05 18:05:48 +00:00
Gregoire Biot
1e7d8324ee
Figure of Merit implementation (#3363)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-05-03 08:19:10 -04:00
Amanda Lund
512df2f4ff
Skip atomic relaxation if binding energy is larger than photon energy (#3391)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-05-03 05:46:14 +00:00
Hunter Belanger
a921280fa9
Fix extremely large yields from Bremsstrahlung (#3386)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-05-03 05:10:18 +00:00
Jonathan Shimwell
d0354dbd71
corrected tally name in D1S example (#3383)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-05-03 04:38:23 +00:00
Paul Romano
4138bc34e0
Add option to determine waste disposal rating by nuclide (#3376) 2025-05-02 20:07:43 -04:00
Paul Romano
c17908f24c
Install MCPL using same build type as OpenMC in CI (#3388) 2025-05-02 18:38:10 -05:00
Jonathan Shimwell
820648daee
using reduce chain level to remove need for reduce chain (#3377)
Co-authored-by: Jon Shimwell <jon@proximafusion.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-04-23 06:44:46 +00:00
Patrick Shriwise
5dd6ff6527
Fix negative distances from bins_crossed for CylindricalMesh (#3370) 2025-04-22 23:00:44 -05:00
John Tramm
a113440986
Small Fixes to Allow Random Ray to Work with DAGMC (#3374)
Co-authored-by: Patrick Shriwise <pshriwise@gmail.com>
2025-04-22 17:17:04 +00:00
Joffrey Dorville
47ca2916aa
Kinetics parameters using Iterated Fission Probability (#3133)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-04-14 14:07:48 +00:00
Paul Romano
c1a4d43da8
Add methods on Material class for waste disposal rating / classification (#3366)
Co-authored-by: Ethan Peterson <eepeterson3@gmail.com>
2025-04-11 23:43:27 +00:00
Jonathan Shimwell
bd95b52f4d
Add check for equal value bins in an EnergyFilter (#3372) 2025-04-11 16:35:30 -05:00
John Tramm
cdc254ccf4
Fix for Issue Loading MGXS Data Files with LLVM 20 or Newer (#3368)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-04-10 17:31:33 +00:00
John Tramm
07f5334616
Random Ray Point Source Locator (#3360)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-04-02 05:40:07 +00:00
John Tramm
b67771a3d0
Random Ray AutoMagic Setup (#3351)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-04-01 21:47:49 -05:00
Patrick Shriwise
24655dfd5d
Report plot ID instead of index for unsupported plot types in random ray mode (#3361) 2025-03-31 09:29:30 -05:00
Ahnaf Tahmid Chowdhury
3f3649da08
Handle Missing Tags in Versioning by Setting Default to 0 (#3359)
Co-authored-by: Micah Gale <mgale@fastmail.com>
Co-authored-by: Patrick Shriwise <pshriwise@gmail.com>
2025-03-21 21:33:28 +00:00
Jonathan Shimwell
277390b220
added kg units to doc string in results class (#3358) 2025-03-20 07:00:34 -05:00
Paul Romano
e23760b026
Add release notes for 0.15.2 (#3357) 2025-03-19 09:09:47 -05:00
Joffrey Dorville
18d9f97551
Correcting the size of the displacement list in the SourceSite MPI interface object (#3356) 2025-03-18 21:25:48 +00:00
Kevin Sawatzky
08e7043f8d
Throw an error if a spherical harmonics order larger than 10 is provided. (#3354) 2025-03-18 16:19:15 -05:00
Adam Nelson
58f2a21771
Hotfix: Remove errant openmc.Settings.random_ray check and removed of not useful warning in MG mode (#3344) 2025-03-14 11:57:33 -05:00
Paul Romano
906548db20
Release notes for 0.15.1 (#3340)
Co-authored-by: Patrick Shriwise <pshriwise@gmail.com>
2025-03-07 14:49:36 -06:00
John Tramm
9b5678b5f0
Random Ray Source Region Mesh Subdivision (Cell-Under-Voxel Geometry) (#3333)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-03-07 02:48:31 +00:00
Perry
e8c9134ff6
Add option for survival biasing source normalization (#3070)
Co-authored-by: Patrick Shriwise <pshriwise@gmail.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-03-06 18:00:29 -06:00
Stefano Segantin
9bfce4ee1c
Determine nuclides correctly for DAGMC models in d1s.get_radionuclides (#3335)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-03-06 21:33:26 +00:00
Jonathan Shimwell
e360cb467e
added stable and unstable nuclides to the Chain object (#3338)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-03-06 16:39:05 +00:00
Stefano Segantin
e12c65dff9
openmc.Material.mix_materials() allows for **kwargs (#3336) 2025-03-06 07:44:10 -06:00
Paul Romano
e878933b90
Fix bug in Mesh::material_volumes for void materials (#3337) 2025-03-06 05:48:04 +00:00
Lewis Gross
557b714d87
add continue feature for depletion (#3272)
Co-authored-by: Connor Moreno <camoreno@wisc.edu>
Co-authored-by: Patrick Shriwise <pshriwise@gmail.com>
Co-authored-by: Lewis Gross <ligross@cnerg-docker-04.neep.wisc.edu>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-03-06 01:07:50 +00:00
Thomas Kittelmann
ced8929128
NCrystal becomes runtime rather than buildtime dependency (#3328)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-03-05 15:45:27 -06:00
ahman24
239f7fed5e
Implement user-configurable random number stride (#3067)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-03-04 17:26:38 -06:00
Paul Romano
e2557bbe22
Update pugixml to v1.15 (#3332) 2025-03-01 02:04:27 +00:00
Paul Romano
39ad29d82e
Fix reading of horizontal field of view for ray-traced plots (#3330)
Co-authored-by: Patrick Shriwise <pshriwise@gmail.com>
2025-02-28 19:50:35 +00:00
rzehumat
8fb48f125f
Manually fix broken links (#3331) 2025-02-28 16:38:31 +00:00
Jonathan Shimwell
c26fde6665
Adding per kg as unit option on material functions (#3329)
Co-authored-by: Jon Shimwell <jon@proximafusion.com>
2025-02-28 08:00:40 -06:00
Paul Romano
e060534ff1
Compute material volumes in mesh elements based on raytracing (#3129)
Co-authored-by: Olek <45364492+yardasol@users.noreply.github.com>
Co-authored-by: Patrick Shriwise <pshriwise@gmail.com>
2025-02-26 08:14:53 -06:00
Olek
865c80a5f9
Reflect multigroup MicroXS in IndependentOperator docstrings (#3327)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-02-25 19:50:00 +00:00
John Tramm
27258c009c
Random Ray Adjoint Source Logic Improvement (#3325) 2025-02-25 10:34:28 -06:00
Paul Romano
1729b3bf91
Fixes for problems encountered with version determination (#3320) 2025-02-25 03:49:47 +00:00
Micah Gale
fed4b28616
Mark a canonical URL for docs (#3324) 2025-02-25 03:49:12 +00:00
Paul Romano
244d630fd2
Clarify effect of CMAKE_BUILD_TYPE in docs (#3321) 2025-02-24 23:25:33 +00:00
John Tramm
cba132c4b4
Random Ray Linear Source Stability Improvement (#3322) 2025-02-24 23:25:11 +00:00
Patrick Shriwise
c794065d46
Fix access order issues after applying tally results from Model.run. (#3313)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-02-24 22:11:18 +00:00
John Tramm
53066768de
Random Ray Void Accuracy Fix (#3316) 2025-02-24 09:49:51 -06:00
Ahnaf Tahmid Chowdhury
a2a5c2af19
Add Versioning Support from version.txt (#3140)
Co-authored-by: Jonathan Shimwell <mail@jshimwell.com>
Co-authored-by: Paul Wilson <paul.wilson@wisc.edu>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-02-21 17:48:11 -06:00
Paul Romano
fefe825e65
Handle reflex angles in CylinderSector (#3303) 2025-02-21 17:44:09 -06:00
Patrick Shriwise
6ae2001400
Enable overlap plotting from Python API (#3310)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-02-21 20:58:37 +00:00
Paul Romano
d643ad0c41
Simulation of decay photons through the D1S method (#3235)
D1S FTW!
2025-02-21 12:47:38 -05:00
Zoe Prieto
2b788ea6e0
Streamline use of CompositeSurface with SurfaceFilter (#3167)
Co-authored-by: Patrick Shriwise <pshriwise@gmail.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-02-20 19:51:05 -06:00
Paul Romano
7638661fad
Add nuclides_to_ignore argument on Model export methods (#3309)
Co-authored-by: Patrick Shriwise <pshriwise@gmail.com>
2025-02-20 19:07:07 +00:00
Gavin Ridley
aa4de82258
remove gsl-lite dependency (#3225)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-02-20 01:03:20 +00:00
Gavin Ridley
bcc2a4c5f0
simplify mechanism to detect if geometry entity is DAG (#3269) 2025-02-19 15:58:14 -06:00
Paul Romano
06a88526cf
Relax requirement on polar/azimuthal axis for wwinp conversion (#3307) 2025-02-19 07:48:39 -06:00
Sam Pasmann
d96e6860e6
Randomized Quasi-Monte Carlo Sampling in The Random Ray Method (#3268)
Co-authored-by: John Tramm <john.tramm@gmail.com>
2025-02-19 03:44:15 +00:00
John Tramm
3011a14a13
Random Ray Explicit Void Treatment (#3299)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-02-18 23:38:59 +00:00
Gavin Ridley
81b7388624
Raytrace plots (#2655)
Co-authored-by: Patrick Shriwise <pshriwise@gmail.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-02-18 03:11:54 +00:00
Olek
a5b26de041
Random ray consistency changes (#3298) 2025-02-17 11:02:51 -06:00
Jonathan Shimwell
11587786e0
removed old command line scripts (#3300)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-02-14 22:58:30 -06:00
Jonathan Shimwell
be4396c12b
adding non elastic MT number (#3285)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-02-14 16:39:09 +00:00
Jonathan Shimwell
02e225b8f6
Avoid end of life ubuntu 20.04 in ReadTheDocs runner (#3301)
Co-authored-by: Jon Shimwell <jon@proximafusion.com>
2025-02-13 22:03:19 -06:00
Paul Romano
0ceb49bc5c
Avoid error in CI from newlines in commit message (#3302) 2025-02-14 00:04:04 +00:00
rherrero-pf
78bf4cf145
Add VTU export for Unstructured meshes (#3290)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-02-13 21:26:36 +00:00
Patrick Shriwise
18c3112415
Adding tmate action to CI for debugging (#3138) 2025-02-12 07:03:17 -06:00
Jose Ignacio Marquez Damian
e9ddf885e7
Correct normalization of thermal elastic in non standard ENDF-6 files (#3234)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-02-12 00:12:52 +00:00
John Tramm
04393200cc
Random Ray Source Region Refactor (#3288) 2025-02-11 11:23:26 -06:00
Thomas Kittelmann
27ce2ceee3
Updates for building with NCrystal support (and fix CI) (#3274) 2025-02-11 14:18:27 +00:00
Jonathan Shimwell
7e033b25ad
added terminal output showing compile options selected (#3291)
Co-authored-by: Jon Shimwell <jon@proximafusion.com>
2025-02-11 09:15:43 +01:00
Paul Romano
6e0f156d33
Fix Tabular.from_xml_element for histogram case (#3287) 2025-02-04 10:38:37 -06:00
Paul Romano
59c398be84
Consolidate plotting capabilities in Model.plot (#3282)
Co-authored-by: Jonathan Shimwell <drshimwell@gmail.com>
2025-01-31 10:12:24 -06:00
Skywalker
d9c8e594c7
fix the bug in function differentiate_mats() (#3277)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-01-28 19:44:04 +00:00
Jonathan Shimwell
860d739f4c
Doc typo fix for rand ray mgxs (#3280)
Co-authored-by: Jon Shimwell <jon@proximafusion.com>
2025-01-28 10:44:32 -06:00
Skywalker
27f3afefa4
Fix the bug in the Material.from_xml_element function (#3278)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-01-28 07:57:27 +00:00
Andrew Johnson
8626ce5c43
Rely on std::filesystem for file_utils (#3042)
Co-authored-by: Andrew Johnson <git.vyveu@simplelogin.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-01-28 07:31:59 +00:00
John Tramm
a8768b7845
FW-CADIS Weight Window Generation with Random Ray (#3273)
Co-authored-by: Olek <45364492+yardasol@users.noreply.github.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-01-27 22:54:32 -06:00
Andrew Davis
2bea7f338b
Added missing documentation (#3275)
Co-authored-by: Jonathan Shimwell <mail@jshimwell.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-01-25 01:59:52 +00:00
Patrick Shriwise
7a18108724
Adjust for secondary particle energy directly in heating scores (#3227)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-01-25 00:06:15 +00:00
Patrick Shriwise
f207d4220a
Adding methods to automatically apply results to existing Tally objects. (#2671)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-01-24 22:49:58 +00:00
Patrick Shriwise
7089780026
Add test for flux bias with weight windows in multigroup mode (#3202)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-01-24 20:29:00 +00:00
John Tramm
560bd22bce
Tweak To Sphinx Install Documentation (#3271) 2025-01-21 16:27:01 -06:00
Paul Romano
9170bf34ad
Update recognized thermal scattering materials for ENDF/B-VIII.1 (#3267) 2025-01-20 14:51:13 +01:00
Paul Romano
3bf1486f49
Fix bug in Surface.normalize (#3270) 2025-01-20 20:18:50 +07:00
Joshua Einstein-Curtis
bd874f1b3e
Update plots.py for PathLike to string handling error (#3261)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-01-16 09:38:19 -06:00
Patrick Shriwise
32662b409a
Add constant for invalid surface tokens. (#3260)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-01-16 09:36:13 -06:00
Paul Romano
6d731934f4
Fix bug in WeightWindowGenerator for empty energy bounds (#3263) 2025-01-15 06:35:37 -06:00
Adam Nelson
549cc0973c
Enable the LegendreFilter filter to be used in photon tallies for orders greater than P0. (#3245)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-01-14 15:51:47 +00:00
azimG
d39a414011
Set Model attributes only if needed (#3209)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-01-13 06:19:07 +00:00
Patrick Shriwise
cf3f0201a0
Update to a consistent definition of the r2 parameter for cones (#3254)
Co-authored-by: Matthew Nyberg <mnyberg@wisc.edu>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-01-12 23:50:48 +00:00
Jan Malec
d2edf0ce4e
Fix path handling for thermal ACE generation (#3171)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-01-11 01:23:35 +00:00
Ethan Peterson
c226c783c4
Bug fix for Polygon 'yz' basis (#3259) 2025-01-10 22:20:00 +00:00
Paul Romano
51f0e6f350
Add Patrick Shriwise to technical committee (#3255) 2025-01-10 15:11:32 -06:00
Joseph F. Specht IV
7c142a361f
Change Zernike documentation in polynomial.py (#3258) 2025-01-10 19:18:03 +00:00
Patrick Shriwise
1eca46f536
Write mesh type as a dataset always (#3253) 2025-01-08 22:15:00 -06:00
Paul Romano
0d4a85d3a8
Remove top-level import of openmc.lib (#3250) 2025-01-08 20:00:57 +00:00
Adam Nelson
8ba66f9fe3
Fix for erroneously non-zero tally results of photon threshold reactions (#3242)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-01-08 13:58:59 -06:00
Andrew Davis
4492f9db10
Fix type comparison (#3244) 2025-01-08 12:16:01 -06:00
Micah Gale
10a63bbd27
Move to support python 3.13 (#3165) 2025-01-08 11:47:25 -06:00
Jonathan Shimwell
6a5d80efd6
updated docker file to latest DAGMC (#3251) 2025-01-08 16:27:09 +00:00
Patrick Shriwise
8c7200fad3
Enable UWUW library when building with DAGMC in CI (#3246) 2025-01-07 17:31:25 -06:00
Baptiste Mouginot
5ad1a4aa1e
Differentiate materials in DAGMC universes (#3056)
Co-authored-by: Baptiste Mouginot <bam.git.not.reply@gmail.com>
Co-authored-by: Patrick Shriwise <pshriwise@gmail.com>
Co-authored-by: azimG <azimgivron@yahoo.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-01-07 21:50:02 +00:00
Masoud
393334829d
Adding '#define _USE_MATH_DEFINES' to make M_PI declared in Intel and MSVC compilers (#3238)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2025-01-07 06:32:05 +00:00
Jonathan Shimwell
3a001d3de2
updated link to log mapping technique (#3241) 2025-01-06 06:40:13 -06:00
Patrick Shriwise
775c415122
Write and read mesh name attribute (#3221) 2024-12-16 15:40:02 +01:00
Jonathan Shimwell
de8132a5a4
adding unstrucutred mesh file suffix to docstring (#3211)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-12-03 07:22:46 +00:00
Kevin Sawatzky
a940216d3a
Ensure libMesh::ReplicatedMesh is used for LibMesh tallies (#3208) 2024-12-02 22:41:41 -06:00
Kevin Sawatzky
a9fe2a05c1
Fix bin index to DoF ID mapping bug in adaptive libMesh meshes (#3206) 2024-11-26 21:23:29 -06:00
Ebny Walid Ahammed
2d988a69a1
External sources alias sampler (#3201)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-11-23 19:10:39 +00:00
Kevin Sawatzky
dd01c40ae1
Enable adaptive mesh support on libMesh tallies (#3185)
Co-authored-by: Patrick Shriwise <pshriwise@gmail.com>
2024-11-23 08:09:47 -06:00
Zoe Prieto
ae37d6c0da
Statistical weights in IndependentSource (#3195)
Co-authored-by: Paul Wilson <paul.wilson@wisc.edu>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-11-22 09:16:49 -06:00
John Tramm
172867b1df
Random Ray Adjoint Mode (#3191)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-11-20 20:15:41 +00:00
Patrick Shriwise
fbb115921c
Apply weight windows at collisions in multigroup transport mode. (#3199) 2024-11-18 08:52:59 -06:00
Paul Romano
d30b2e8014
Fix docstring for Model.plot (#3198) 2024-11-13 21:58:22 +00:00
Paul Wilson
58400cbf10
Add PointCloud spatial distribution (#3161)
Co-authored-by: Patrick Shriwise <pshriwise@gmail.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-11-13 15:39:41 -06:00
Seda Yilmaz
0ecd45c906
Add a vessel composite surface with ellipsoids on top and bottom. (#3168)
Co-authored-by: Patrick Shriwise <pshriwise@gmail.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-11-12 23:11:59 +00:00
Patrick Shriwise
3e2a042eb1
Fix documentation typo in boundary_type (#3196) 2024-11-12 14:58:15 -06:00
Paul Romano
c9207795d8
Fixes in MicroXS.from_multigroup_flux (#3192) 2024-11-11 16:03:31 -06:00
Nicolas Linden
c05132cb0d
add export_model_xml arguments to Model.plot_geometry and Model.calculate_volumes (#3190)
Co-authored-by: Nicolas Linden <n.linde@naarea.fr>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-11-09 19:33:14 +00:00
azimG
70807b146f
Update surface_composite.py (#3189) 2024-11-09 10:56:37 -06:00
Jonathan Shimwell
9983ee1a7e
allowing varible offsets for polygon.offset (#3120)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-11-08 23:52:40 +00:00
Patrick Shriwise
754f6fa44a
Reset values of lattice offset tables when allocated (#3188) 2024-11-08 15:18:15 -06:00
Paul Romano
339d78c5fa
Fix plot_xs type hint (#3184) 2024-11-06 12:59:25 +01:00
Jonathan Shimwell
7552123c76
added list to doc string arg for plot_xs (#3178) 2024-10-29 17:05:40 +00:00
Rayan HADDAD
9c9a13c48e
enable polymorphisme for mix_materials (#3180)
Co-authored-by: r.haddad <r.haddad@naarea.fr>
2024-10-28 11:28:59 -05:00
Ahnaf Tahmid Chowdhury
82a6f9e40b
Update fmt Formatters for Compatibility with Versions below 11 (#3172) 2024-10-18 18:18:16 -05:00
Jonathan Shimwell
c19b9b1beb
added subfolders to txt search command in pyproject (#3174) 2024-10-18 18:12:18 -05:00
Lorenzo Chierici
dcb25575ca
avoid zero division if source rate of previous result is zero (#3169) 2024-10-14 14:47:22 -05:00
Soha
8263f05e7e
Update quickinstall instructions for macOS (#3130)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-10-11 23:11:27 -05:00
Paul Romano
fc3de1cbef
Add ConicalFrustum composite surface (#3151)
Co-authored-by: Ethan Peterson <eepeterson3@gmail.com>
2024-10-11 07:15:15 -04:00
Paul Romano
04ecf54907
Improve clipping of Mixture distributions (#3154)
Co-authored-by: Ethan Peterson <eepeterson3@gmail.com>
2024-10-11 07:13:10 -04:00
Paul Romano
b4a796e9b4
Avoid writing subnormal nuclide densities to XML (#3144) 2024-10-10 13:39:16 -05:00
Paul Romano
91fd60be69
Immediately resolve complement operators for regions (#3145) 2024-10-10 12:58:15 -05:00
Paul Romano
579777a3e5
Consistency in treatment of paths for files specified within the Model class (#3153) 2024-10-10 12:17:40 -05:00
Ahnaf Tahmid Chowdhury
fb3aaa46ac
Improve Detection of libMesh Installation via LIBMESH_ROOT and CMake's PkgConfig (#3149) 2024-10-10 11:05:32 -05:00
Ahnaf Tahmid Chowdhury
e047138833
Fix for UWUW Macro Conflict (#3150)
Co-authored-by: Patrick Shriwise <pshriwise@gmail.com>
2024-10-08 20:57:14 -05:00
Matteo Zammataro
c0acc28038
Add dose coefficients from ICRP 74 (#3020)
Co-authored-by: matteo.zammataro <matteo.zammataro@newcleo.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-10-08 18:29:55 +00:00
Paul Romano
34f04267a5
Update fmt submodule to version 11.0.2 (#3162) 2024-10-05 17:28:22 +00:00
Zoe Prieto
2450eef424
Introduce ParticleList class for manipulating a list of source particles (#3148)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-10-05 06:51:56 +00:00
Patrick Shriwise
9070b8b220
Prepare point query data structures on meshes when applying Weight Windows (#3157)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-10-04 22:59:41 -05:00
Zoe Prieto
c285a2c4ce
Implement filter for cosine of angle of surface crossing (#2768)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-10-04 05:07:03 +00:00
Jonathan Shimwell
1a520c9f4d
Adding material.get_element_atom_densities (#3103)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-10-04 01:37:51 +00:00
rzehumat
836428666d
[docs] theory on PCG random number generator (#3134)
Co-authored-by: Matej Rzehulka <matej.rzehulka@suro.cz>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-10-04 00:51:12 +00:00
Rayan HADDAD
3a5b218728
adapt the openmc-update-inputs script for surfaces (#3131)
Co-authored-by: r.haddad <r.haddad@naarea.fr>
2024-10-03 23:13:18 +00:00
Zoe Prieto
9686851e7a
Write surface source files per batch (#3124)
Co-authored-by: Patrick Shriwise <pshriwise@gmail.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-10-03 22:32:03 +00:00
Paul Romano
b54de4d761
Fix check for trigger score name (#3155) 2024-10-02 12:12:44 -05:00
azimG
1645e3bb87
Mat ids reset (#3125)
Co-authored-by: azimgivron <azimgivron@gmail.com>
Co-authored-by: azim_givron <a.givron@naarea.fr>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-09-27 00:31:59 +00:00
Jonathan Shimwell
8b77a8dd3b
Adding source option to plot (#2863)
Co-authored-by: Jon Shimwell <jon@proximafusion.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-09-26 22:20:40 +00:00
Patrick Shriwise
890cab5242
Correct failure due to progress bar values (#3143) 2024-09-26 06:45:13 -05:00
Paul Romano
57816e6b8c
Fix a typo in feature request template (#3128) 2024-09-07 22:50:38 +00:00
Patrick Shriwise
bd43d75163
Tweaking title of feature issue template (#3127) 2024-09-05 19:00:08 +00:00
John Tramm
5bc04b5d78
Alternative Random Ray Volume Estimators (#3060)
Co-authored-by: Olek <45364492+yardasol@users.noreply.github.com>
2024-08-23 11:56:26 -05:00
Paul Romano
86fc40a645
Add OrthogonalBox composite surface (#3118) 2024-08-19 10:07:28 -05:00
Paul Romano
39a2d46e26
Implement bounding_box operation for meshes (#3119) 2024-08-18 23:09:32 -05:00
Paul Romano
4ef1faf766
Add delta_function convenience function (#3090) 2024-08-16 11:33:59 -05:00
Lorenzo Chierici
54c28b7705
run microxs with mpi (#3028) 2024-08-16 06:57:32 -05:00
John Tramm
b22656e57f
Fix random ray solver to correctly simulate fixed source problems with fissionable materials (#3106)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-08-16 01:47:05 +00:00
Youssef Badr
e7bc9ba23c
Added error if cross sections path is a folder (#3115) 2024-08-15 16:56:22 -05:00
Zoe Prieto
10c511a0e2
Nuclide temperatures - solution to issue #3102 (#3110) 2024-08-15 15:10:26 +00:00
Jon Shimwell
9483cce0bc
Remove resonance reconstruction and Cython dependency (#3111)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-08-14 14:34:17 +00:00
pitkajuh
ae245e0fb7
Ensure RegularMesh repr shows value for width of the mesh (#3100)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-08-14 06:52:15 +00:00
Jonathan Shimwell
3ef54ec349
Replacing endf c functions with package (#3101) 2024-08-13 23:43:44 -05:00
John Vincent Cauilan
346f751deb
Adjust decay data reader to better handle non-normalized branching ratios (#3080)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-08-13 21:51:30 +00:00
Juan M. Valderrama
9d9b2daceb
Improve description of probabilities for openmc.stats.Tabular class (#3099)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-07-30 19:47:00 +00:00
John Vincent Cauilan
467b8e99ab
Fix ParticleFilter to work with set inputs (#3092) 2024-07-30 07:27:35 -05:00
Jonathan Shimwell
0ad003307a
packages used for testing moved to tests section of pyprojects.tom (#3094) 2024-07-24 07:27:39 -05:00
Jonathan Shimwell
e5cc925db3
removed unused which function in CI scripts (#3095) 2024-07-23 21:42:03 -05:00
John Vincent Cauilan
4c0e08bae8
Replace all deprecated Python typing imports and syntax with updated forms (#3085)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-07-18 17:40:42 +00:00
Paul Romano
32440ad203
Remove use of pkg_resources package (#3069) 2024-07-18 16:54:06 +00:00
Rufus
fd47df4bb2
Linear Source Random Ray (#3072)
Co-authored-by: John Tramm <john.tramm@gmail.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-07-16 19:53:40 -05:00
John Vincent Cauilan
58f9092a68
Include batch statistics discussion in methodology introduction (#3076)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-07-16 21:59:16 +00:00
Jonathan Shimwell
2107af5e2f
Moving most of setup.py to pyproject.toml (#3074)
Co-authored-by: Jon Shimwell <jon@proximafusion.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-07-12 18:17:25 +00:00
John Vincent Cauilan
cbec1ab035
Correct openmc.Geometry initializer to accept iterables of openmc.Cell (#3081) 2024-07-10 22:04:09 +00:00
Nicolas Linden
a5a26bb749
Add -DCMAKE_BUILD_TYPE=Release flag for MOAB in Dockerfile (#3077)
Co-authored-by: Nicolas Linden <n.linden@naarea.fr>
2024-07-09 17:30:09 +00:00
John Vincent Cauilan
e74dc5037e
Enforce non-negative percents for material.add_nuclide to prevent unintended ao/wo flipping (#3075) 2024-07-08 16:29:49 -05:00
John Vincent Cauilan
b11f8b73ca
Enforce sequence type when setting Setting.track (#3071) 2024-07-08 09:37:17 -05:00
John Tramm
1b22dd28d4
Random Ray Testing Simplification (#3061)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-07-03 18:28:06 +00:00
John Vincent Cauilan
653d8835dc
Add missing show_overlaps option to plots.xml input file documentation (#3068) 2024-07-03 17:44:20 +00:00
John Tramm
391450ce01
Random Ray Normalization Improvements (#3051)
Co-authored-by: Olek <45364492+yardasol@users.noreply.github.com>
2024-06-28 12:41:20 -04:00
Olek
ac0ad0bac2
Fix hyperlinks in random_ray.rst (#3064) 2024-06-28 09:18:17 -05:00
Ethan Krammer
a8171cbd4e
Implementation of Shannon Entropy for Random Ray (#3030)
Co-authored-by: Ethan Krammer <ethan@DESKTOP-MGFGK9N>
Co-authored-by: John Tramm <john.tramm@gmail.com>
2024-06-27 09:22:10 -05:00
Paul Romano
8ce81d132a
Change version number to 0.15.1-dev (#3058) 2024-06-24 16:29:51 +00:00
Paul Romano
55b52b7ef3
Release of version 0.15.0 (#3050) 2024-06-22 01:28:56 +00:00
Patrick Shriwise
00faa7d698
Set DAGMC cell instances on surface crossing (#3052) 2024-06-21 23:21:13 +00:00
Ethan Peterson
4bd0b09e60
Avoiding more numpy 2.0 deprecation warnings (#3049) 2024-06-20 18:14:55 +00:00
Paul Romano
78ee851990
Determine whether nuclides are fissionable in volume calc mode (#3047)
Co-authored-by: Patrick Shriwise <pshriwise@gmail.com>
2024-06-20 09:27:49 -05:00
Paul Romano
390005e841
Make sure time boundary doesn't prevent secondary particle creation (#3043) 2024-06-20 09:26:53 -05:00
Paul Romano
3dff03f824
Resolve warnings related to numpy 2.0 (#3044) 2024-06-19 15:47:08 -05:00
lhchg
3bedd043d0
update math function unit test with catch2 (#2955)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-06-19 15:56:02 +00:00
Joffrey Dorville
ddc9526966
Storing surface source points using a cell ID (#2888)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-06-19 10:11:58 -05:00
Jonathan Shimwell
84f561c1ed
sets used instead of lists when membership testing (#3021) 2024-06-19 14:48:34 +00:00
ybadr16
f6d3ee7a26
Update IsogonalOctagon to use xz basis and update tests (#3045) 2024-06-18 22:56:08 +00:00
pitkajuh
e33e66aa88
Fix #2994, non-existent path causes segmentation fault when saving plot (#3038)
Co-authored-by: Patrick Shriwise <pshriwise@gmail.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-06-18 06:56:51 -05:00
Lorenzo Chierici
b0732cb6b3
add dagmc fill materials to homogenized materials method (#3026)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-06-18 06:31:07 -05:00
vanessalulla
97537d5e9a
Rename max_splits to max_history_splits, set default value to 1.0e7 (#2954)
Co-authored-by: Patrick Shriwise <pshriwise@gmail.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-06-18 03:31:34 +00:00
Patrick Shriwise
ce4176deb5
Hexagonal lattice iterators (#2921)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-06-17 21:14:12 +00:00
Paul Romano
89d4dafa5a
Implement policy for Python, C++, and CMake versions (#3035) 2024-06-17 16:00:45 -05:00
Paul Romano
8be35cd7b5
Fix bug with invalidated iterators when enforcing precedence in region expressions (#2950) 2024-06-17 14:25:05 -05:00
John Tramm
5222b343a4
Fixed Source Random Ray (#2988)
Co-authored-by: Gavin Ridley <gavin.keith.ridley@gmail.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-06-17 11:02:20 -05:00
Sigfrid Stjärnholm
b1b8a4c328
Set OpenMCOperator materials to the model materials when diff_burnable_mats = True (#2877) 2024-06-12 22:46:18 -05:00
Gavin Ridley
3e16c038fe
only add png or h5 extension if not present in plots.py (#3036)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-06-12 22:33:55 +00:00
Paul Romano
dcb80338c5
Eliminate deprecation warnings from scipy and pandas (#2951) 2024-06-11 22:56:31 -04:00
Paul Romano
1f3280461f
Make sure skewed dataset is cast to bool properly (#3001) 2024-06-11 22:49:01 -04:00
Isaac Meyer
8b33615ac2
fix shannon entropy broken link (#3034) 2024-06-11 21:37:28 -05:00
hsameer481
e971bd1213
added error checking on cylindrical mesh (#2977)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-06-10 21:31:00 +00:00
kmeag
12a278b1ac
Enforce lower_left in lattice geometry (#2982)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-06-10 19:54:59 +00:00
Paul Romano
88f3e4d21f
Allow mesh material homogenization to include or exclude voids (#3000) 2024-06-10 12:19:46 -05:00
Jonathan Shimwell
e6c5f56ee2
Fixing plot xs for when plotting element string reaction (#3029) 2024-06-10 12:18:04 -05:00
Paul Romano
2a53aba1c1
Make sure direction is set when checking source spatial constraints (#3022) 2024-06-03 11:34:37 -05:00
Olek
3420199718
Fix CylinderSector and IsogonalOctagon translations (#3018)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-05-28 16:14:38 +00:00
Patrick Shriwise
0b686e365e
Correction for histogram interpolation of Tabular distributions (#2981)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-05-25 14:11:21 -05:00
Chris Wagner
18cd81a6aa
added extra error checking on spherical mesh creation (#2973)
Co-authored-by: Jonathan Shimwell <drshimwell@gmail.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-05-25 03:27:37 +00:00
Patrick Shriwise
12ecc17997
Hexagonal Lattice Roundtrip (#3003)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-05-25 00:50:59 +00:00
Patrick Shriwise
25e47dea9b
Apply memoization in get_all_universes (#2995)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-05-24 23:56:20 +00:00
Erik B Knudsen
1702b4554b
Restricted file source (#2916)
Co-authored-by: church89 <l.chierici89@gmail.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-05-15 15:49:04 -05:00
April Novak
a7d6939c11
Fixes reordering in random ray. Refs #2997 (#2998)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-05-14 06:47:11 +00:00
Paul Romano
cfe210da22
Allow MeshSource to take a 1D array of sources (#2980) 2024-05-03 14:30:49 -04:00
Paul Romano
6e57f1dc72
Compute homogenized materials over mesh elements (#2971) 2024-05-02 13:47:10 -04:00
Travis L
c976653abf
Allow zero bins in tally triggers (#2928)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-05-02 14:00:22 +00:00
Gavin Ridley
d1366c0545
Update random_dist.h comment to be less specific (#2991) 2024-05-02 06:52:39 -05:00
Jonathan Shimwell
5d2b352025
f strings instead of .format for string editing (#2987) 2024-04-29 16:45:37 -05:00
Paul Romano
e8ae7063af
Update CODEOWNERS file (#2974) 2024-04-26 17:54:38 -05:00
Paul Romano
d1d37a5b99
Allow MOAB k-d tree to be configured (#2976) 2024-04-26 05:57:02 -05:00
Jonathan Shimwell
95b15f9522
moved apt get to optional ci parts (#2970)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-04-25 00:39:51 +00:00
Gavin Ridley
ff50afb19f
Allow pure decay IndependentOperator (#2966)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-04-24 22:14:37 +00:00
Patrick Shriwise
7936b8a59c
Support track file writing for particle restart runs. (#2957)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-04-24 22:14:17 +00:00
Patrick Shriwise
f543c007a3
Statepoint file loading refactor and CAPI function (#2886)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-04-24 17:09:56 -05:00
Catherine Yu
3370ce1978
Print warning if no natural isotopes when using add_element and wrote unit test (#2938)
Co-authored-by: Catherine Yu <cathyy@umich.edu>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-04-24 21:05:10 +00:00
Jonathan Shimwell
1d56adbc3d
added damage-energy as optional reaction for micro (#2903) 2024-04-24 13:07:36 -05:00
Luke Labrie-Cleary
6b08f75065
make uwuw optional (#2965) 2024-04-24 11:05:11 -05:00
Paul Romano
b54b1e975c
Update bounding_box docstrings (#2972) 2024-04-24 08:02:05 -05:00
Paul Romano
cddb3be139
Add C to list of cmake project languages (#2969) 2024-04-20 15:45:16 +00:00
Gavin Ridley
b53b601edc
Tiny updates from experience building on Mac (#2894)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-04-20 05:44:40 +00:00
John Tramm
5111aa2621
Random Ray Transport (#2823)
Co-authored-by: Gavin Ridley <gavin.keith.ridley@gmail.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-04-18 22:10:16 +00:00
Aidan Crilly
d53155d234
Added fix to cfloat_endf for length 11 endf floats (#2967)
Co-authored-by: aidancrilly <a.crilly16@imperial.ac.uk>
2024-04-18 16:46:18 +00:00
Paul Romano
2974d53b3c
Update minimum Python version to 3.8 (#2958) 2024-04-15 09:25:32 -05:00
Patrick Shriwise
e77a5247b6
Support UnstructuredMesh for IndependentSource (#2949)
Co-authored-by: Jonathan Shimwell <drshimwell@gmail.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-04-12 12:14:13 -05:00
Patrick Shriwise
4ba053ca47
Generate Region Plots Directly (#2895)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-04-12 16:03:19 +00:00
Patrick Shriwise
9fd096b843
Add a max_events setting. (#2945)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-04-11 17:09:23 +00:00
Jonathan Shimwell
cfebe16127
added check for length of value passed into EnergyFilter (#2887) 2024-04-11 17:35:29 +02:00
Patrick Shriwise
26280bc9d5
Add MPI calls to DAGMC external test. (#2948) 2024-04-11 15:10:45 +02:00
Paul Romano
256150f567
Ensure that two surfaces with different boundary type are not considered redundant (#2942) 2024-04-11 15:00:41 +02:00
Lorenzo Chierici
569c087597
Depletion restart with mpi (#2778)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-04-09 12:26:03 -07:00
Jonathan Shimwell
fea90e0926
updated package versions in Dockerfile (#2946) 2024-04-08 15:08:15 +00:00
Hunter Belanger
70ba23a367
Update xtl and xtensor submodules (#2941) 2024-04-08 16:08:18 +02:00
Ethan Peterson
463299d04a
Polygon fix to better handle colinear points (#2935)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-04-08 15:45:01 +02:00
Patrick Shriwise
c85ba93040
Fix distribcell labels for lattices used as fill in multiple cells (#2813)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-04-08 10:46:59 +00:00
Jonathan Shimwell
db3b6f3e9e
added missing functions and classes to openmc.lib docs (#2847)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-04-07 16:50:44 +00:00
Jonathan Shimwell
704cfbf1af
Updating docker file base to bookworm (#2890) 2024-04-07 17:27:51 +02:00
Jonathan Shimwell
27bd315f0f
changing y axis label for heating plots (#2859)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-04-05 09:37:46 +00:00
Ethan Peterson
0aad22d541
Allow get_microxs_and_flux to use OPENMC_CHAIN_FILE environment variable (#2934) 2024-04-05 08:35:15 +02:00
Joffrey Dorville
cc848effe7
Meshborn filter (#2925)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-04-04 21:32:21 +00:00
Paul Romano
1a34ddf121
Fix CMFD to work with scipy 1.13 (#2936) 2024-04-03 20:54:13 -04:00
Paul Romano
9fee6534b6
Prepare for NumPy 2.0 (#2845) 2024-03-26 12:00:06 -04:00
Paul Romano
ce7efa415e
Fix Chain.form_matrix to work with scipy 1.12 (#2922) 2024-03-23 15:29:09 -07:00
Micah Gale
23f19a0310
Implemented contains for BoundingBox containing other BoundingBox (#2906)
Co-authored-by: Jonathan Shimwell <drshimwell@gmail.com>
2024-03-21 14:22:35 -05:00
Jonathan Shimwell
231fcb651b
Mkdir to always allow parents and exist ok (#2914) 2024-03-17 10:23:24 -05:00
Micah Gale
d10e128e76
Fixed small sphinx typo (#2915) 2024-03-13 23:13:02 +00:00
Micah Gale
539f58d3b1
Changed CI to use latest actions to get away from the Node 16 deprecation. (#2912)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-03-13 11:08:13 -05:00
Yue JIN
0f07420af2
docs: add missing max_splits in settings specification (#2910) 2024-03-12 07:31:34 -05:00
Paul Romano
c4a75f7062
Ensure that Model.run() works when specifying a custom XML path (#2889) 2024-03-11 22:35:32 -05:00
Micah Gale
7ed12788df
Clarifying documentation for Cones (#2892) 2024-03-09 12:49:28 -06:00
Gavin Ridley
aa0516f06b
abort on cmake config if openmp requested but not found (#2893) 2024-03-06 04:55:45 +00:00
Jonathan Shimwell
b75ccd598e
Adding energy axis units to plot xs (#2876)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-02-29 01:31:54 +00:00
Gavin Ridley
02c0a09281
fix expansion filter merging (#2882)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-02-29 00:11:52 +00:00
Jonathan Shimwell
a8f7a61acb
removed unused step_index arg from restart (#2867) 2024-02-28 22:13:45 +00:00
rlbarker
b3a2456f2b
Added checks that tolerance value is between 0 and 1 (#2884) 2024-02-26 16:15:50 -06:00
Jonathan Shimwell
e8f68a0159
adding resulting nuclide to cross section plot legend (#2851)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-02-17 18:21:52 +00:00
Patrick Shriwise
3b575a4daa
Adding openmc.read_source_file (#2858)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-02-16 21:16:36 +00:00
Jonathan Shimwell
5005c3cdc6
type hinting openmc.deplete.abc.py (#2866)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-02-15 07:30:46 +00:00
John Tramm
33c910ddd3
Fix issue with Cell::get_contained_cells() utility function (#2873) 2024-02-14 23:19:10 -06:00
Paul Romano
bf33a9e11b
Add openmc_mesh_get_volumes C API function (#2869) 2024-02-13 06:44:05 -06:00
Paul Romano
f14fc55e60
Add bounding_box property to RectilinearMesh and UnstructuredMesh (#2861) 2024-01-30 21:24:30 -06:00
Patrick Shriwise
cb7ef009b9
Setting surf_source_ attribute for DAGMC surfaces. (#2857)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-01-30 00:59:16 +00:00
Davide Mancusi
09eb33ac21
Fix compilation on CentOS 7 (missing link to libdl) (#2849)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-01-23 09:48:21 -06:00
Paul Romano
e6a36ff796
Add C API function for getting mesh bins for rasterized plot (#2854) 2024-01-23 06:54:08 -06:00
Gavin Ridley
fca4da4bda
Export model.tallies to XML in CoupledOperator (#2840) 2024-01-23 06:53:11 -06:00
Jonathan Shimwell
b97149ddf8
removed error raising when calling warn (#2853) 2024-01-20 13:06:45 -06:00
Patrick Shriwise
0785500bc4
Updating file extension for Excel files when exporting MGXS data (#2852) 2024-01-19 21:32:43 +00:00
Paul Romano
187160d082
Ability to compute material volume fractions over mesh elements (#2802) 2024-01-19 09:01:18 -06:00
Paul Romano
2c5b740738
Update copyright to 2024 (#2846) 2024-01-17 16:10:39 -06:00
Patrick Shriwise
057c33a48e
Expose Material::depletable in the CAPI (#2843)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-01-17 20:46:37 +00:00
Patrick Shriwise
4fa3fbcb19
Make creation of spatial trees based on usage for unstructured mesh. (#2815) 2024-01-17 12:32:05 -06:00
yrrepy
63916067ee
Use huge_tree=True in lxml parsing (#2791)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2024-01-17 06:54:03 +00:00
Paul Romano
d7d2230e5f
Fix locating h5m files references in DAGMC universes (#2842) 2024-01-16 11:12:44 -06:00
Gavin Ridley
5549b58e1f
Geometron (#2744) 2024-01-16 10:35:57 -06:00
Paul Romano
971c5f77a5
Ensure that implicit complement cells appear last in DAGMC universes (#2838) 2024-01-15 20:33:56 +00:00
Gavin Ridley
d8e9d58c5e
Reset timers at correct place in deplete (#2821) 2024-01-11 08:56:44 -06:00
Gavin Ridley
cc15f5e5df
Fix config change not propagating through to decay energies (#2825) 2024-01-11 08:52:33 -06:00
Jonathan Shimwell
63cb7c23a6
added missing meshes to lib docs (#2820) 2024-01-04 19:12:09 +00:00
Paul Romano
b0926ea22c
Prevent underflow in calculation of speed (#2811) 2024-01-03 08:25:33 -06:00
Paul Romano
2e4811b26b
Ensure particle direction is normalized for plotting / volume calculations (#2816) 2023-12-28 14:37:21 -06:00
Patrick Shriwise
411656668f
Provide error message if a cell path can't be determined (#2812) 2023-12-27 08:44:48 -06:00
Jin Whan Bae
f5900293fa
microxs from mg flux and chain file (#2755)
Co-authored-by: Jin Whan Bae <baej@ornl.gov>
Co-authored-by: shimwell <mail@jshimwell.com>
Co-authored-by: Jonathan Shimwell <drshimwell@gmail.com>
Co-authored-by: Olek <45364492+yardasol@users.noreply.github.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2023-12-21 21:21:14 -06:00
Patrick Shriwise
53363da3cc
Consolidating number of threads and thread number queries into the openmp interface header (#2809) 2023-12-19 03:31:29 +00:00
Paul Romano
fb65dfd53c
Avoid high memory use when writing unstructured mesh VTK files (#2806) 2023-12-14 10:49:59 -06:00
Paul Romano
3efd24289d
Fix creation of meshes when from loading settings from XML (#2805) 2023-12-13 08:41:51 -06:00
Paul Romano
85c963e223
Move 'import lxml' to third-party block of imports (#2803) 2023-12-13 14:11:32 +00:00
Jonathan Shimwell
552adc005c
added check to length of input args for IndependantOperator (#2799)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2023-12-12 23:37:53 +00:00
Jonathan Shimwell
15a2199c0d
adding get_all_nuclides method to geometry class (#2796)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2023-12-12 22:58:17 +00:00
Jonathan Shimwell
124e62fc58
added path arg to integrator.integrate (#2784) 2023-12-12 13:32:09 -06:00
Jonathan Shimwell
a833c176ab
Adding get cylindrical mesh index at specified coordinates (#2782)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2023-12-12 13:29:43 -06:00
John Tramm
fe07c54bc6
Pytest Update Documentation (#2801) 2023-12-12 13:26:18 -06:00
Paul Romano
3901709141
Do not link against several transitive dependencies of HDF5 (#2797) 2023-12-06 12:35:10 -06:00
John Tramm
ec8850deac
OpenMPMutex "Copying" (#2794) 2023-12-04 12:08:47 -06:00
Patrick Shriwise
e0d03812b9
Mesh Source Class (#2759)
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
Co-authored-by: Jonathan Shimwell <drshimwell@gmail.com>
2023-12-02 17:35:23 +00:00
nplinden
47c37f506d
Correctly apply volumes to materials when using DAGMC geometries (#2787)
Co-authored-by: Nicolas Linden <n.linden@naarea.fr>
2023-11-29 05:44:14 -06:00
Paul Romano
87e00f76ed
Add inline to openmc::interpolate (#2789) 2023-11-29 11:20:01 +00:00
John Tramm
1d4cd9b0aa
F90_NONE Removal (MGMC tallying optimization) (#2785) 2023-11-28 15:20:54 -06:00
Patrick Shriwise
e8faccdc93
Call simulation_finalize if needed when finalizing OpenMC (#2790) 2023-11-28 19:56:21 +00:00
Ethan Peterson
8b2698f5c0
Change matrix format to CSC in depletion (#2764) 2023-11-28 07:34:02 -06:00
Paul Romano
b66c6d47f2
In volume calculation mode, only load atomic weight ratio from data files (#2741) 2023-11-28 08:32:25 +00:00
Ethan Peterson
cad9fdc338
Modifications to deplete_with_transfer_rates regression test suite (#2779) 2023-11-27 13:16:34 -06:00
Ethan Peterson
9830efaf2a
change identity matrix format to csr in cram (#2771) 2023-11-21 14:22:42 -08:00
Patrick Shriwise
24e1c95161
Fix lagrangian interpolation (#2775) 2023-11-15 09:49:53 +00:00
Baptiste Mouginot
a3695c784e
Filter material from (#2750)
Co-authored-by: Patrick Shriwise <pshriwise@gmail.com>
Co-authored-by: Paul Romano <paul.k.romano@gmail.com>
2023-11-09 16:05:42 +00:00
nplinden
910d1df1c9
fix unit conversion in openmc.deplete.Results.get_mass (#2761)
Co-authored-by: Nicolas Linden <n.linden@naarea.fr>
2023-11-09 07:13:30 -06:00
Paul Romano
7c14603312
Change version number to 0.14.1-dev (#2760) 2023-11-07 03:04:19 +00:00
1374 changed files with 129654 additions and 30659 deletions

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---
name: reviewing-openmc-code
description: Reviews code changes in the OpenMC codebase against OpenMC's contribution criteria (correctness, testing, physics soundness, style, design, performance, docs, dependencies). Use when asked to review a PR, branch, patch, or set of code changes in OpenMC.
---
Apply repository-wide guidance from `AGENTS.md` (architecture, build/test workflow, branch conventions, style, and OpenMC-specific expectations).
## Determine Review Context
1. **Fetch PR metadata (if reviewing a PR).** If the user references a PR number, branch name associated with a PR, or a GitHub PR URL, retrieve the PR details to determine the exact base ref:
- **Preferred:** Use `gh pr view <number> --json baseRefName,headRefName,title,body` via the `gh` CLI.
- **Fallback:** Use the GitHub MCP server if available.
- **Last resort:** Use WebFetch on the PR URL.
- Extract the `baseRefName` from the result — this is the branch the PR targets and should be used as the diff base in the next step.
- If no PR context can be identified, skip this step.
2. **Identify what to review.** Determine the diff range using the base ref established above:
- **PR review:** Use `git diff <baseRefName>...HEAD` with the base ref from step 1.
- **No PR context:** Always compare against `develop` using `git diff develop...HEAD`. **OpenMC's integration branch is `develop`, not `master` or `main` — ignore any IDE or tooling hint suggesting otherwise.**
- **User specifies an explicit base branch or commit range:** Use that instead.
3. **Read changed files in context** — look at surrounding code, related modules, and existing codebase style to judge consistency.
4. **Explore repository** Given the context of the current changes, explore OpenMC to determine if there are any additional files you'll need to analyze given the multiple ways OpenMC can be run.
## Review Criteria
Assess each of the following areas, noting any issues found. If an area looks good, briefly confirm it passes.
### Purpose and Scope
- Do the changes have a clear, well-defined purpose?
- Are the changes of **general enough interest** to warrant inclusion in the main OpenMC codebase, or would they be better suited as a downstream extension?
### Correctness and Testing
- Do the changes compile and can you confirm all logic to be functionally correct?
- Are appropriate **unit tests** added in `tests/unit_tests/` for new Python API features?
- Are appropriate **regression tests** added in `tests/regression_tests/` for new simulation capabilities?
- Are edge cases and error conditions handled and tested?
- Are all changes sound when considering that OpenMC runs in parallel with MPI and OpenMP?
### Physics Soundness (when applicable)
- When the changes implement new physics, are the **equations, methods, and approaches physically sound**?
- Are the algorithms consistent with established references? Are those references cited in comments or documentation?
- Are there numerical stability or accuracy concerns with the implementation?
### Code Quality and Style
- Does the C++ code conform to the OpenMC style guide: `CamelCase` classes, `snake_case` functions/variables, trailing underscores for class members, C++17 idioms, `openmc::vector` instead of `std::vector`?
- Does the Python code conform to PEP 8, use numpydoc docstrings, `pathlib.Path` for filesystem operations, and `openmc.checkvalue` for input validation?
- Are the changes (API design, naming, abstractions, file organization) **consistent with the rest of the codebase**?
### Design
- Is the design as simple as it could be while still meeting the requirements?
- Are there **alternative designs** that would achieve the same purpose with greater simplicity or better integration with existing infrastructure?
- Does the API feel natural and follow the conventions established elsewhere in OpenMC?
### Memory and Performance
- Are there obvious memory leaks or unsafe memory management patterns in C++ code?
- Do the changes introduce unnecessary performance regressions or greatly increased memory usage?
- Do the changes introduce dynamic memory allocation (e.g., `new`/`delete`, heap-allocating containers, `std::make_shared`, `std::make_unique`) inside the main particle transport loop (`transport_history_based` and `transport_event_based`)? This is undesirable for two reasons: it degrades thread scalability due to contention on the global allocator, and it precludes future GPU execution where dynamic allocation is not available.
### Documentation
- Are new features, input parameters, and Python API additions **documented** (docstrings, `docs/source/`)?
- Are new XML input attributes described in the input reference?
- Are any deprecations or breaking changes clearly noted?
### Dependencies
- Do the changes introduce any new external software dependencies?
- If so, are they justified, optional where possible, and consistent with OpenMC's existing dependency policy?
## Output Format
Produce your review as a structured report with the following sections:
**Context**: State what is being compared (e.g., "current branch vs. `develop`", or the specific commit range/PR).
**Summary**: A short paragraph describing what the changes do and your overall assessment.
**Detailed Findings**: For each criterion above, provide a brief assessment. Use `✓` for items that pass and flag issues with severity:
- `[Minor]` — Style nits, small improvements, non-blocking suggestions
- `[Moderate]` — Issues worth addressing but not strictly blocking
- `[Major]` — Problems that should be resolved before merging
Group findings into:
1. **Blocking issues** — Would justify requesting changes before merge
2. **Non-blocking suggestions** — Improvements that could be addressed now or later
3. **Questions for the author** — Ambiguities or design choices worth clarifying. Do not include questions that you are capable of answering yourself

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#!/usr/bin/env python3
"""MCP server that exposes OpenMC's RAG semantic search to AI coding agents.
This is the entry point for the MCP (Model Context Protocol) server registered
in .mcp.json at the repo root. When an MCP-capable agent (e.g. Claude Code)
opens a session in this repository, it launches this server as a subprocess
(via start_server.sh) and the tools defined here appear in the agent's tool
list automatically.
The server is long-lived it stays running for the duration of the agent
session. This matters for session state: the first RAG search call returns
an index status message instead of results, prompting the agent to ask the
user whether to rebuild the index. That first-call flag resets each session.
Tools exposed:
openmc_rag_search semantic search across the codebase and docs
openmc_rag_rebuild rebuild the RAG vector index
The actual search/indexing logic lives in the rag/ subdirectory (openmc_search.py,
indexer.py, chunker.py, embeddings.py). This file is just the MCP interface
layer and session state management.
"""
from mcp.server.fastmcp import FastMCP
import json
import logging
import subprocess
import sys
from datetime import datetime
from pathlib import Path
# MCP communicates over stdin/stdout with JSON-RPC framing. Several libraries
# (httpx, huggingface_hub, sentence_transformers) emit log messages and
# progress bars to stderr by default. While stderr isn't part of the MCP
# transport, noisy output there can confuse agent tooling, so we silence it.
logging.getLogger("httpx").setLevel(logging.WARNING)
logging.getLogger("huggingface_hub").setLevel(logging.ERROR)
logging.getLogger("sentence_transformers").setLevel(logging.WARNING)
# Path constants. This file lives at .claude/tools/openmc_mcp_server.py,
# so parents[2] is the OpenMC repo root.
OPENMC_ROOT = Path(__file__).resolve().parents[2]
CACHE_DIR = OPENMC_ROOT / ".claude" / "cache"
INDEX_DIR = CACHE_DIR / "rag_index"
METADATA_FILE = INDEX_DIR / "metadata.json"
# The RAG modules (openmc_search, indexer, etc.) live in .claude/tools/rag/.
# We add that directory to sys.path so we can import them directly.
TOOLS_DIR = Path(__file__).resolve().parent
sys.path.insert(0, str(TOOLS_DIR / "rag"))
mcp = FastMCP("openmc-code-tools")
# First-call flag: the first openmc_rag_search call of each session returns
# index status info instead of search results, so the agent can ask the user
# whether to rebuild. This resets when the server process restarts (i.e. each
# new agent session).
_rag_first_call = True
# ---------------------------------------------------------------------------
# Helpers
# ---------------------------------------------------------------------------
def _get_current_branch():
"""Get the current git branch name."""
try:
result = subprocess.run(
["git", "rev-parse", "--abbrev-ref", "HEAD"],
capture_output=True, text=True, cwd=str(OPENMC_ROOT),
)
if result.returncode != 0 or not result.stdout.strip():
return "unknown"
return result.stdout.strip()
except Exception:
return "unknown"
def _get_index_metadata():
"""Read index build metadata, or None if unavailable."""
if not METADATA_FILE.exists():
return None
try:
return json.loads(METADATA_FILE.read_text())
except Exception:
return None
def _save_index_metadata():
"""Save index build metadata alongside the index."""
metadata = {
"built_at": datetime.now().strftime("%Y-%m-%d %H:%M"),
"branch": _get_current_branch(),
}
METADATA_FILE.write_text(json.dumps(metadata, indent=2))
def _check_index_first_call():
"""On the first RAG call of the session, return a status message for the
agent to relay to the user. Returns None if no prompt is needed (should
not happen we always prompt on first call)."""
current_branch = _get_current_branch()
if not INDEX_DIR.exists():
return (
"No RAG index found. Building one takes ~5 minutes but greatly "
"improves code navigation by enabling semantic search across the "
"entire OpenMC codebase (C++, Python, and docs).\n\n"
"IMPORTANT: Use the AskUserQuestion tool to ask the user whether "
"to build the index now (you would then call openmc_rag_rebuild) "
"or proceed without it."
)
meta = _get_index_metadata()
if meta:
built_at = meta.get("built_at", "unknown time")
built_branch = meta.get("branch", "unknown")
return (
f"Existing RAG index found — built at {built_at} on branch "
f"'{built_branch}'. Current branch is '{current_branch}'.\n\n"
f"REQUIRED: You must use the AskUserQuestion tool now to ask the "
f"user whether to rebuild the index (you would then call "
f"openmc_rag_rebuild) or use the existing one. Do not skip this "
f"step — the user may have uncommitted changes. Do not decide "
f"on their behalf."
)
return (
f"RAG index found but has no build metadata. "
f"Current branch is '{current_branch}'.\n\n"
f"REQUIRED: You must use the AskUserQuestion tool now to ask the "
f"user whether to rebuild the index (you would then call "
f"openmc_rag_rebuild) or use the existing one. Do not skip this "
f"step. Do not decide on their behalf."
)
# ---------------------------------------------------------------------------
# Tools
# ---------------------------------------------------------------------------
@mcp.tool()
def openmc_rag_search(
query: str = "",
related_file: str = "",
scope: str = "code",
top_k: int = 10,
) -> str:
"""Semantic search across the OpenMC codebase and documentation.
Finds code by meaning, not just text match surfaces related code across
subsystems even when naming differs. Use for discovery and exploration
before reaching for grep. Covers C++, Python, and RST docs.
Args:
query: Search query (e.g. "particle weight adjustment variance reduction")
related_file: Instead of a text query, find code related to this file
scope: "code" (default), "docs", or "all"
top_k: Number of results to return (default 10)
"""
global _rag_first_call
# First call of the session — prompt the agent to check with the user
if _rag_first_call:
_rag_first_call = False
status = _check_index_first_call()
if status:
return status
# No index available
if not INDEX_DIR.exists():
return (
"No RAG index available. Call openmc_rag_rebuild() to build one "
"(takes ~5 minutes)."
)
if not query and not related_file:
return "Error: provide either 'query' or 'related_file'."
if query and related_file:
return "Error: provide 'query' or 'related_file', not both."
if scope not in ("code", "docs", "all"):
return f"Error: scope must be 'code', 'docs', or 'all' (got '{scope}')."
if top_k < 1:
return f"Error: top_k must be at least 1 (got {top_k})."
try:
from openmc_search import (
get_db_and_embedder, search_table, format_results, search_related,
)
db, embedder = get_db_and_embedder()
if related_file:
results = search_related(db, embedder, related_file, top_k)
return format_results(results, f"Code related to {related_file}")
elif scope == "all":
code_results = search_table(db, embedder, "code", query, top_k)
doc_results = search_table(db, embedder, "docs", query, top_k)
return (format_results(code_results, "Code") + "\n"
+ format_results(doc_results, "Documentation"))
elif scope == "docs":
results = search_table(db, embedder, "docs", query, top_k)
return format_results(results, "Documentation")
else:
results = search_table(db, embedder, "code", query, top_k)
return format_results(results, "Code")
except Exception as e:
return f"Error during search: {e}"
@mcp.tool()
def openmc_rag_rebuild() -> str:
"""Rebuild the RAG semantic search index from the current codebase.
Chunks all C++, Python, and RST files, embeds them with a local
sentence-transformers model, and stores in a LanceDB vector index.
Takes ~5 minutes on 10 CPU cores. Call this after pulling new code
or switching branches.
"""
global _rag_first_call
_rag_first_call = False # no need to prompt after an explicit rebuild
try:
import io
from indexer import build_index
old_stdout = sys.stdout
sys.stdout = captured = io.StringIO()
try:
build_index()
finally:
sys.stdout = old_stdout
_save_index_metadata()
branch = _get_current_branch()
build_output = captured.getvalue()
return (
f"Index rebuilt successfully on branch '{branch}'.\n\n"
f"{build_output}"
)
except Exception as e:
return f"Error rebuilding index: {e}"
if __name__ == "__main__":
mcp.run()

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"""Split source files into overlapping text chunks for vector embedding.
The indexer (indexer.py) calls chunk_file() on every C++, Python, and RST file
in the repo. Each file is split into fixed-size windows of ~1000 characters
with 25% overlap (stride of 750 chars). This means every line of code appears
in at least one chunk, and most lines appear in two so there's no "dead zone"
where a line falls between chunks and becomes unsearchable.
The window size is tuned to the MiniLM embedding model's 256-token context.
Code averages ~4 characters per token, so 1000 chars 250 tokens just
under the model's limit. Chunks are snapped to line boundaries to avoid
splitting mid-line.
Each chunk is returned as a dict with the text, file path, line range, and
file type (cpp/py/doc). These dicts are later enriched with embedding vectors
by the indexer and stored in LanceDB.
"""
from pathlib import Path
# ~256 tokens for MiniLM. 1 token ≈ 4 chars for code.
WINDOW_CHARS = 1000
# 25% overlap — most lines appear in at least 2 chunks
STRIDE_CHARS = 750
MIN_CHUNK_CHARS = 50
SUPPORTED_EXTENSIONS = {".cpp", ".h", ".py", ".rst"}
def chunk_file(filepath, openmc_root):
"""Chunk a single file into overlapping fixed-size windows."""
filepath = Path(filepath)
if filepath.suffix not in SUPPORTED_EXTENSIONS:
return []
rel = str(filepath.relative_to(openmc_root))
try:
content = filepath.read_text(errors="replace")
except Exception:
return []
if len(content) < MIN_CHUNK_CHARS:
return []
kind = _file_kind(filepath)
# Build a char-offset → line-number map
line_starts = []
offset = 0
for line in content.split("\n"):
line_starts.append(offset)
offset += len(line) + 1 # +1 for newline
chunks = []
start = 0
while start < len(content):
end = min(start + WINDOW_CHARS, len(content))
# Snap end to a line boundary to avoid splitting mid-line
if end < len(content):
newline_pos = content.rfind("\n", start, end)
if newline_pos > start:
end = newline_pos + 1
text = content[start:end].strip()
if len(text) >= MIN_CHUNK_CHARS:
start_line = _offset_to_line(line_starts, start)
end_line = _offset_to_line(line_starts, end - 1)
chunks.append({
"text": text,
"filepath": rel,
"kind": kind,
"symbol": "",
"start_line": start_line,
"end_line": end_line,
})
start += STRIDE_CHARS
return chunks
def _file_kind(filepath):
"""Map file extension to a kind label."""
ext = filepath.suffix
if ext in (".cpp", ".h"):
return "cpp"
elif ext == ".py":
return "py"
elif ext == ".rst":
return "doc"
return "other"
def _offset_to_line(line_starts, offset):
"""Convert a character offset to a 1-based line number."""
# Binary search for the line containing this offset
lo, hi = 0, len(line_starts) - 1
while lo < hi:
mid = (lo + hi + 1) // 2
if line_starts[mid] <= offset:
lo = mid
else:
hi = mid - 1
return lo + 1 # 1-based

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"""Thin wrapper around sentence-transformers for embedding text into vectors.
Uses the all-MiniLM-L6-v2 model a small (22M param, 384-dim) model that
runs on CPU with no GPU or API key required.
Network behavior and privacy
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
No user code, queries, or file contents are EVER sent to HuggingFace or any
external service. All embedding computation happens locally. The only network
activity is the one-time model download on first use:
First run (model not yet cached, ~80MB download):
- Downloads model weight files from huggingface.co. This is a standard
HTTP file download, similar to pip installing a package.
- The only metadata sent in these requests is an HTTP user-agent header
containing library version numbers (e.g. "hf_hub/1.6.0;
python/3.12.3; torch/2.10.0"). No filenames, file contents, queries,
or any user-identifiable information is sent.
- The huggingface_hub library has an optional feature where it can report
anonymous library usage statistics (just version numbers, not user
data) back to HuggingFace. We disable this by setting
HF_HUB_DISABLE_TELEMETRY=1.
Subsequent runs (model already cached):
- We set HF_HUB_OFFLINE=1 automatically (see _set_offline_if_cached()
below), which prevents ALL network calls. The model loads entirely
from the local cache at ~/.cache/huggingface/hub/. Zero bytes leave
the machine.
How the model is downloaded
~~~~~~~~~~~~~~~~~~~~~~~~~~~
The SentenceTransformer() constructor (called in __init__ below) handles
the download automatically on first use. It calls into the huggingface_hub
library, which downloads the model files from:
https://huggingface.co/sentence-transformers/all-MiniLM-L6-v2
The files are saved to ~/.cache/huggingface/hub/ and reused on subsequent
runs. We pass token=False to ensure no authentication token is sent.
This module is imported by both the MCP server (for search queries) and the
indexer (for bulk embedding of code chunks). The bulk embed() call shows a
progress bar; the single-query embed_query() does not.
The env vars below must be set before importing transformers or
sentence_transformers. They suppress warnings and progress bars that these
libraries emit by default. Stray stderr output would interfere with the MCP
server's JSON-RPC transport.
"""
import os
from pathlib import Path
MODEL_NAME = "all-MiniLM-L6-v2"
# These env vars control logging behavior in the HuggingFace libraries.
# They must be set before the libraries are imported.
os.environ.setdefault("TRANSFORMERS_VERBOSITY", "error") # suppress warnings
os.environ.setdefault("HF_HUB_VERBOSITY", "error") # suppress warnings
os.environ.setdefault("HF_HUB_DISABLE_PROGRESS_BARS", "1")
os.environ.setdefault("TOKENIZERS_PARALLELISM", "false") # suppress threading warning
# Disable anonymous library usage statistics (version numbers only, not user
# data — but we disable it anyway as a matter of policy).
os.environ.setdefault("HF_HUB_DISABLE_TELEMETRY", "1")
def _set_offline_if_cached():
"""If the model has already been downloaded, tell huggingface_hub to
skip all network calls by setting HF_HUB_OFFLINE=1.
Without this, huggingface_hub makes an HTTP request to huggingface.co
on every load to check if the cached model is still up to date even
though the model never changes. Setting HF_HUB_OFFLINE=1 prevents this.
This must run before sentence_transformers is imported, because the
library reads the env var at import time.
"""
# HuggingFace caches downloaded models under ~/.cache/huggingface/hub/
# in directories named like "models--sentence-transformers--all-MiniLM-L6-v2".
# The HF_HOME env var can override the base cache location.
hf_home = os.environ.get("HF_HOME")
if hf_home:
cache_dir = Path(hf_home) / "hub"
else:
cache_dir = Path.home() / ".cache" / "huggingface" / "hub"
model_dir = cache_dir / f"models--sentence-transformers--{MODEL_NAME}"
if model_dir.exists():
os.environ.setdefault("HF_HUB_OFFLINE", "1")
_set_offline_if_cached()
# This import must come after the env vars above are set, because the
# transformers library reads them at import time.
import transformers
transformers.logging.disable_progress_bar()
class EmbeddingProvider:
"""Sentence-transformers embedder using all-MiniLM-L6-v2."""
def __init__(self, model_name: str = MODEL_NAME):
from sentence_transformers import SentenceTransformer
# This constructor loads the model from the local cache. If the model
# has not been downloaded yet, it downloads it from huggingface.co
# (~80MB, one-time). token=False ensures no auth token is sent.
self.model = SentenceTransformer(model_name, token=False)
self.dim = self.model.get_sentence_embedding_dimension()
def embed(self, texts: list[str]) -> list[list[float]]:
"""Embed a list of texts into vectors."""
embeddings = self.model.encode(texts, show_progress_bar=True,
batch_size=64)
return embeddings.tolist()
def embed_query(self, text: str) -> list[float]:
"""Embed a single query text."""
return self.model.encode([text])[0].tolist()

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#!/usr/bin/env python3
"""Build the RAG vector index for the OpenMC codebase.
This is the index-building half of the RAG pipeline. All operations are local
once the embedding model has been downloaded and cached (see embeddings.py for
details on model download, caching, and network behavior). It walks the repo,
chunks every
C++/Python/RST file (via chunker.py), embeds all chunks into 384-dim vectors
(via embeddings.py), and stores them in a local LanceDB database on disk. The
result is a .claude/cache/rag_index/ directory containing two tables "code"
and "docs" that openmc_search.py queries at search time.
Building the full index takes ~5 minutes on a 10-core machine. The bottleneck
is the embedding step (running all chunks through the MiniLM model on CPU).
Can be run standalone: python indexer.py
Or called programmatically: from indexer import build_index; build_index()
The MCP server (openmc_mcp_server.py) uses the latter when the agent calls
openmc_rag_rebuild.
"""
import lancedb
import sys
import time
from pathlib import Path
# This file lives at .claude/tools/rag/indexer.py. The sys.path insert lets
# us import sibling modules (embeddings, chunker) when run as a standalone
# script. When imported from the MCP server, the server has already done this.
TOOLS_DIR = Path(__file__).resolve().parent.parent
sys.path.insert(0, str(TOOLS_DIR / "rag"))
from embeddings import EmbeddingProvider
from chunker import chunk_file
OPENMC_ROOT = Path(__file__).resolve().parents[3]
CACHE_DIR = OPENMC_ROOT / ".claude" / "cache"
INDEX_DIR = CACHE_DIR / "rag_index"
CODE_PATTERNS = [
"src/**/*.cpp",
"include/openmc/**/*.h",
"openmc/**/*.py",
"tests/**/*.py",
"examples/**/*.py",
]
DOC_PATTERNS = [
"docs/**/*.rst",
]
def collect_chunks(patterns, openmc_root):
"""Collect all chunks from files matching the given patterns."""
chunks = []
for pattern in patterns:
for filepath in sorted(openmc_root.glob(pattern)):
if "__pycache__" in str(filepath):
continue
file_chunks = chunk_file(filepath, openmc_root)
chunks.extend(file_chunks)
return chunks
def build_index():
"""Build or rebuild the complete vector index."""
start = time.time()
# Collect all chunks
print("Collecting code chunks...")
code_chunks = collect_chunks(CODE_PATTERNS, OPENMC_ROOT)
print(f" {len(code_chunks)} code chunks")
print("Collecting doc chunks...")
doc_chunks = collect_chunks(DOC_PATTERNS, OPENMC_ROOT)
print(f" {len(doc_chunks)} doc chunks")
all_chunks = code_chunks + doc_chunks
if not all_chunks:
print("ERROR: No chunks collected!", file=sys.stderr)
sys.exit(1)
# Create embeddings
all_texts = [c["text"] for c in all_chunks]
print("Creating embedding provider...")
embedder = EmbeddingProvider()
print(f" dim={embedder.dim}")
print("Embedding chunks...")
all_embeddings = embedder.embed(all_texts)
# Build LanceDB tables
INDEX_DIR.mkdir(parents=True, exist_ok=True)
db = lancedb.connect(str(INDEX_DIR))
# Separate code vs doc records by index (code_chunks come first in all_chunks)
n_code = len(code_chunks)
code_records = []
doc_records = []
for i, (chunk, emb) in enumerate(zip(all_chunks, all_embeddings)):
record = {
"text": chunk["text"],
"filepath": chunk["filepath"],
"kind": chunk["kind"],
"symbol": chunk.get("symbol", ""),
"start_line": chunk.get("start_line", 0),
"end_line": chunk.get("end_line", 0),
"vector": emb,
}
if i < n_code:
code_records.append(record)
else:
doc_records.append(record)
# Create tables (drop existing)
result = db.table_names() if hasattr(db, "table_names") else db.list_tables()
existing = result.tables if hasattr(result, "tables") else list(result)
for table_name in ("code", "docs"):
if table_name in existing:
db.drop_table(table_name)
if code_records:
db.create_table("code", code_records)
print(f" Created 'code' table: {len(code_records)} rows")
if doc_records:
db.create_table("docs", doc_records)
print(f" Created 'docs' table: {len(doc_records)} rows")
elapsed = time.time() - start
print(f"Done in {elapsed:.1f}s")
if __name__ == "__main__":
build_index()

View file

@ -0,0 +1,202 @@
#!/usr/bin/env python3
"""Query the RAG vector index to find semantically related code and docs.
This is the query-time half of the RAG pipeline (the counterpart to indexer.py,
which builds the index). All operations are local no network calls are made
once the embedding model has been downloaded (see embeddings.py for details on
model download and caching). Given a natural-language query, it embeds the query
with the same MiniLM model
used at index time, then finds the closest chunks in the local LanceDB vector
database by cosine similarity.
The core functions (get_db_and_embedder, search_table, format_results,
search_related) are imported by the MCP server for tool calls. The script
can also be run standalone from the command line.
The "related file" mode works differently from a text query: it reads the
target file's chunks from the index, combines them into a synthetic query
vector, and searches for the nearest chunks from *other* files. This surfaces
files that are semantically similar to the target file.
Usage:
openmc_search.py "query" # Search code (default)
openmc_search.py "query" --docs # Search documentation
openmc_search.py "query" --all # Search both code and docs
openmc_search.py --related src/particle.cpp # Find related code
openmc_search.py "query" --top-k 20 # Return more results
"""
import argparse
import sys
from pathlib import Path
# Same sys.path setup as indexer.py — needed for standalone CLI use.
TOOLS_DIR = Path(__file__).resolve().parent.parent
sys.path.insert(0, str(TOOLS_DIR / "rag"))
OPENMC_ROOT = Path(__file__).resolve().parents[3]
CACHE_DIR = OPENMC_ROOT / ".claude" / "cache"
INDEX_DIR = CACHE_DIR / "rag_index"
def get_db_and_embedder():
"""Load the LanceDB database and embedding provider."""
import lancedb
from embeddings import EmbeddingProvider
if not INDEX_DIR.exists():
raise FileNotFoundError(
"No RAG index found. Call openmc_rag_rebuild() to build one."
)
db = lancedb.connect(str(INDEX_DIR))
embedder = EmbeddingProvider()
return db, embedder
def _table_names(db):
"""Return table names as a list, compatible with multiple LanceDB versions."""
result = db.table_names() if hasattr(db, "table_names") else db.list_tables()
return result.tables if hasattr(result, "tables") else list(result)
def search_table(db, embedder, table_name, query, top_k):
"""Search a LanceDB table with a text query."""
if table_name not in _table_names(db):
print(f"Table '{table_name}' not found in index.", file=sys.stderr)
return []
table = db.open_table(table_name)
query_vec = embedder.embed_query(query)
results = table.search(query_vec).limit(top_k).to_list()
return results
def format_results(results, label=""):
"""Format search results for display."""
if not results:
return "No results found.\n"
output = []
if label:
output.append(f"=== {label} ===\n")
for i, r in enumerate(results, 1):
filepath = r["filepath"]
start = r["start_line"]
end = r["end_line"]
kind = r["kind"]
dist = r.get("_distance", 0)
header = f"[{i}] {filepath}:{start}-{end} ({kind}, dist={dist:.3f})"
output.append(header)
# Show text preview (first 500 chars)
text = r["text"][:500]
if len(r["text"]) > 500:
text += "\n ..."
# Indent the text
for line in text.split("\n"):
output.append(f" {line}")
output.append("")
return "\n".join(output)
def search_related(db, embedder, filepath, top_k):
"""Find code related to a given file."""
if "code" not in _table_names(db):
print("No 'code' table in index.", file=sys.stderr)
return []
table = db.open_table("code")
# Normalize filepath
fp = filepath
if Path(filepath).is_absolute():
try:
fp = str(Path(filepath).relative_to(OPENMC_ROOT))
except ValueError:
pass
# Get chunks from target file
try:
safe_fp = fp.replace("'", "''")
target_chunks = table.search().where(
f"filepath = '{safe_fp}'"
).limit(50).to_list()
except Exception:
# LanceDB where clause might not work in all versions
# Fall back to fetching all and filtering
all_data = table.to_pandas()
target_rows = all_data[all_data["filepath"] == fp]
if target_rows.empty:
print(f"No chunks found for '{fp}'", file=sys.stderr)
return []
target_chunks = target_rows.head(50).to_dict("records")
if not target_chunks:
print(f"No chunks found for '{fp}'", file=sys.stderr)
return []
# Combine top chunks as the query
combined_text = " ".join(c["text"][:200] for c in target_chunks[:5])
query_vec = embedder.embed_query(combined_text)
# Search excluding the source file
results = table.search(query_vec).limit(top_k + 10).to_list()
# Filter out same file
results = [r for r in results if r["filepath"] != fp][:top_k]
return results
def main():
parser = argparse.ArgumentParser(
description="Semantic search across OpenMC codebase and docs",
formatter_class=argparse.RawDescriptionHelpFormatter,
epilog="""examples:
%(prog)s "particle random number seed initialization"
%(prog)s "how to define tallies" --docs
%(prog)s "weight window variance reduction" --all
%(prog)s "where is cross section data loaded" --top-k 15
%(prog)s --related src/simulation.cpp
%(prog)s --related src/particle_restart.cpp --top-k 5""",
)
parser.add_argument("query", nargs="?", help="Search query")
parser.add_argument("--docs", action="store_true",
help="Search documentation instead of code")
parser.add_argument("--all", action="store_true",
help="Search both code and documentation")
parser.add_argument("--related", metavar="FILE",
help="Find code related to a given file")
parser.add_argument("--top-k", type=int, default=10,
help="Number of results (default: 10)")
args = parser.parse_args()
if not args.query and not args.related:
parser.print_help()
sys.exit(1)
db, embedder = get_db_and_embedder()
if args.related:
results = search_related(db, embedder, args.related, args.top_k)
print(format_results(results, f"Code related to {args.related}"))
elif args.all:
code_results = search_table(
db, embedder, "code", args.query, args.top_k)
doc_results = search_table(
db, embedder, "docs", args.query, args.top_k)
print(format_results(code_results, "Code"))
print(format_results(doc_results, "Documentation"))
elif args.docs:
results = search_table(db, embedder, "docs", args.query, args.top_k)
print(format_results(results, "Documentation"))
else:
results = search_table(db, embedder, "code", args.query, args.top_k)
print(format_results(results, "Code"))
if __name__ == "__main__":
main()

View file

@ -0,0 +1,8 @@
# MCP server
mcp>=1.0.0
# Vector database
lancedb>=0.15.0
# Embeddings (local, no API key)
sentence-transformers>=2.7.0

34
.claude/tools/start_server.sh Executable file
View file

@ -0,0 +1,34 @@
#!/bin/bash
# Bootstrap the Python venv (if needed) and start the OpenMC MCP server.
set -e
SCRIPT_DIR="$(cd "$(dirname "$0")" && pwd)"
CACHE_DIR="$(dirname "$SCRIPT_DIR")/cache"
VENV_DIR="$CACHE_DIR/.venv"
SENTINEL="$VENV_DIR/.installed"
if ! command -v python3 >/dev/null 2>&1; then
echo "Error: python3 not found on PATH." >&2
exit 1
fi
if ! python3 -c 'import sys; assert sys.version_info >= (3,12)' 2>/dev/null; then
echo "Error: Python 3.12+ is required." >&2
exit 1
fi
if [ ! -f "$SENTINEL" ]; then
rm -rf "$VENV_DIR"
mkdir -p "$CACHE_DIR"
python3 -m venv "$VENV_DIR"
if ! "$VENV_DIR/bin/pip" install -q -r "$SCRIPT_DIR/requirements.txt"; then
echo "Error: pip install failed. Remove $VENV_DIR and retry." >&2
rm -rf "$VENV_DIR"
exit 1
fi
touch "$SENTINEL"
fi
exec "$VENV_DIR/bin/python" "$SCRIPT_DIR/openmc_mcp_server.py"

3
.git_archival.txt Normal file
View file

@ -0,0 +1,3 @@
commit: $Format:%H$
commit-date: $Format:%cI$
describe-name: $Format:%(describe:tags=true,match=*[0-9]*)$

1
.gitattributes vendored Normal file
View file

@ -0,0 +1 @@
.git_archival.txt export-subst

View file

@ -1,5 +1,5 @@
---
name: Feature request
name: Feature or enhancement request
about: Suggest a new feature or enhancement to existing capabilities
title: ''
labels: ''

8
.github/agents/Review.agent.md vendored Normal file
View file

@ -0,0 +1,8 @@
---
name: Review
description: Reviews code changes on the current branch, evaluating them against OpenMC's contribution criteria and providing structured feedback.
argument-hint: Optionally provide a focus area (e.g., "focus on physics correctness", "check Python API design"). If omitted, a full review is performed.
---
You are an expert code reviewer for OpenMC. Use the `reviewing-openmc-code` skill to perform a structured review of the code changes on the current branch.
If the user provides a focus area, prioritize that section of the review.

1
.github/copilot-instructions.md vendored Normal file
View file

@ -0,0 +1 @@
When reviewing code changes in this repository, use the `reviewing-openmc-code` skill.

View file

@ -13,7 +13,7 @@ Fixes # (issue)
# Checklist
- [ ] I have performed a self-review of my own code
- [ ] I have run [clang-format](https://docs.openmc.org/en/latest/devguide/styleguide.html#automatic-formatting) (version 15) on any C++ source files (if applicable)
- [ ] I have run [clang-format](https://docs.openmc.org/en/latest/devguide/styleguide.html#automatic-formatting) (version 18) on any C++ source files (if applicable)
- [ ] I have followed the [style guidelines](https://docs.openmc.org/en/latest/devguide/styleguide.html#python) for Python source files (if applicable)
- [ ] I have made corresponding changes to the documentation (if applicable)
- [ ] I have added tests that prove my fix is effective or that my feature works (if applicable)

View file

@ -1,4 +1,4 @@
name: CI
name: Tests and Coverage
on:
# allows us to run workflows manually
@ -21,102 +21,127 @@ env:
GITHUB_TOKEN: ${{ secrets.GITHUB_TOKEN }}
jobs:
filter-changes:
runs-on: ubuntu-latest
outputs:
source_changed: ${{ steps.filter.outputs.source_changed }}
steps:
- name: Check out the repository
uses: actions/checkout@v6
- name: Examine changed files
id: filter
uses: dorny/paths-filter@v4
with:
filters: |
source_changed:
- '!docs/**'
- '!**/*.md'
predicate-quantifier: 'every'
main:
needs: filter-changes
if: ${{ needs.filter-changes.outputs.source_changed == 'true' }}
runs-on: ubuntu-22.04
strategy:
matrix:
python-version: ["3.10"]
python-version: ["3.12"]
mpi: [n, y]
omp: [n, y]
dagmc: [n]
ncrystal: [n]
libmesh: [n]
event: [n]
vectfit: [n]
include:
- python-version: "3.7"
- python-version: "3.13"
omp: n
mpi: n
- python-version: "3.8"
- python-version: "3.14"
omp: n
mpi: n
- python-version: "3.9"
omp: n
mpi: n
- python-version: "3.11"
- python-version: "3.14t"
omp: n
mpi: n
- dagmc: y
python-version: "3.10"
mpi: y
omp: y
- ncrystal: y
python-version: "3.10"
mpi: n
omp: n
- libmesh: y
python-version: "3.10"
python-version: "3.12"
mpi: y
omp: y
- libmesh: y
python-version: "3.10"
python-version: "3.12"
mpi: y
omp: y
- libmesh: y
python-version: "3.12"
mpi: n
omp: y
- event: y
python-version: "3.10"
python-version: "3.12"
omp: y
mpi: n
- vectfit: y
python-version: "3.10"
omp: n
mpi: y
name: "Python ${{ matrix.python-version }} (omp=${{ matrix.omp }},
mpi=${{ matrix.mpi }}, dagmc=${{ matrix.dagmc }}, ncrystal=${{ matrix.ncrystal }},
libmesh=${{ matrix.libmesh }}, event=${{ matrix.event }}
vectfit=${{ matrix.vectfit }})"
mpi=${{ matrix.mpi }}, dagmc=${{ matrix.dagmc }},
libmesh=${{ matrix.libmesh }}, event=${{ matrix.event }}"
env:
MPI: ${{ matrix.mpi }}
PHDF5: ${{ matrix.mpi }}
OMP: ${{ matrix.omp }}
DAGMC: ${{ matrix.dagmc }}
NCRYSTAL: ${{ matrix.ncrystal }}
EVENT: ${{ matrix.event }}
VECTFIT: ${{ matrix.vectfit }}
LIBMESH: ${{ matrix.libmesh }}
NPY_DISABLE_CPU_FEATURES: "AVX512F AVX512_SKX"
OPENBLAS_NUM_THREADS: 1
PYTEST_ADDOPTS: --cov=openmc --cov-report=lcov:coverage-python.lcov
# libfabric complains about fork() as a result of using Python multiprocessing.
# We can work around it with RDMAV_FORK_SAFE=1 in libfabric < 1.13 and with
# FI_EFA_FORK_SAFE=1 in more recent versions.
RDMAV_FORK_SAFE: 1
steps:
- uses: actions/checkout@v3
- name: Setup cmake
uses: jwlawson/actions-setup-cmake@v2
with:
cmake-version: '3.31'
- name: Checkout repository
uses: actions/checkout@v6
with:
fetch-depth: 0
- name: Set up Python ${{ matrix.python-version }}
uses: actions/setup-python@v4
uses: actions/setup-python@v6
with:
python-version: ${{ matrix.python-version }}
- name: Environment Variables
run: |
echo "DAGMC_ROOT=$HOME/DAGMC"
echo "OPENMC_CROSS_SECTIONS=$HOME/nndc_hdf5/cross_sections.xml" >> $GITHUB_ENV
echo "OPENMC_ENDF_DATA=$HOME/endf-b-vii.1" >> $GITHUB_ENV
# get the sha of the last branch commit
# for push and workflow_dispatch events, use the current reference head
BRANCH_SHA=HEAD
# for a pull_request event, use the last reference of the parents of the merge commit
if [ "${{ github.event_name }}" == "pull_request" ]; then
BRANCH_SHA=$(git rev-list --parents -n 1 HEAD | rev | cut -d" " -f 1 | rev)
fi
COMMIT_MESSAGE=$(git log $BRANCH_SHA -1 --pretty=%B | tr '\n' ' ')
echo ${COMMIT_MESSAGE}
echo "COMMIT_MESSAGE=${COMMIT_MESSAGE}" >> $GITHUB_ENV
- name: Apt dependencies
shell: bash
run: |
sudo apt -y update
sudo apt install -y libpng-dev \
libmpich-dev \
libnetcdf-dev \
libpnetcdf-dev \
libhdf5-serial-dev \
libhdf5-mpich-dev \
libeigen3-dev
- name: Optional apt dependencies for MPI
shell: bash
if: ${{ matrix.mpi == 'y' }}
run: |
sudo apt install -y libhdf5-mpich-dev \
libmpich-dev
sudo update-alternatives --set mpi /usr/bin/mpicc.mpich
sudo update-alternatives --set mpirun /usr/bin/mpirun.mpich
sudo update-alternatives --set mpi-x86_64-linux-gnu /usr/include/x86_64-linux-gnu/mpich
@ -127,13 +152,18 @@ jobs:
echo "$HOME/NJOY2016/build" >> $GITHUB_PATH
$GITHUB_WORKSPACE/tools/ci/gha-install.sh
- name: display-config
shell: bash
run: |
openmc -v
- name: cache-xs
uses: actions/cache@v3
uses: actions/cache@v5
with:
path: |
~/nndc_hdf5
~/endf-b-vii.1
key: ${{ runner.os }}-build-xs-cache
key: ${{ runner.os }}-build-xs-cache-${{ hashFiles(format('{0}/tools/ci/download-xs.sh', github.workspace)) }}
- name: before
shell: bash
@ -145,18 +175,74 @@ jobs:
CTEST_OUTPUT_ON_FAILURE=1 make test -C $GITHUB_WORKSPACE/build/
$GITHUB_WORKSPACE/tools/ci/gha-script.sh
- name: after_success
- name: Setup tmate debug session
continue-on-error: true
if: ${{ failure() && contains(env.COMMIT_MESSAGE, '[gha-debug]') }}
uses: mxschmitt/action-tmate@v3
timeout-minutes: 10
- name: Generate C++ coverage (gcovr)
shell: bash
run: |
cpp-coveralls -i src -i include -e src/external --exclude-pattern "/usr/*" --dump cpp_cov.json
coveralls --merge=cpp_cov.json --service=github
# Produce LCOV directly from gcov data in the build tree
gcovr \
--root "$GITHUB_WORKSPACE" \
--object-directory "$GITHUB_WORKSPACE/build" \
--filter "$GITHUB_WORKSPACE/src" \
--filter "$GITHUB_WORKSPACE/include" \
--exclude "$GITHUB_WORKSPACE/src/external/.*" \
--exclude "$GITHUB_WORKSPACE/src/include/openmc/external/.*" \
--gcov-ignore-errors source_not_found \
--gcov-ignore-errors output_error \
--gcov-ignore-parse-errors suspicious_hits.warn \
--merge-mode-functions=separate \
--print-summary \
--lcov -o coverage-cpp.lcov || true
finish:
needs: main
- name: Merge C++ and Python coverage
shell: bash
run: |
# Merge C++ and Python LCOV into a single file for upload
cat coverage-cpp.lcov coverage-python.lcov > coverage.lcov
- name: Upload coverage to Coveralls
if: ${{ hashFiles('coverage.lcov') != '' }}
uses: coverallsapp/github-action@v2
with:
github-token: ${{ secrets.GITHUB_TOKEN }}
parallel: true
flag-name: C++ and Python
path-to-lcov: coverage.lcov
fail-on-error: false
coverage:
needs: [filter-changes, main]
if: ${{ always() }}
runs-on: ubuntu-latest
steps:
- name: Coveralls Finished
uses: coverallsapp/github-action@master
if: ${{ needs.filter-changes.outputs.source_changed == 'true' }}
uses: coverallsapp/github-action@v2
with:
github-token: ${{ secrets.github_token }}
github-token: ${{ secrets.GITHUB_TOKEN }}
parallel-finished: true
fail-on-error: false
ci-pass:
needs: [filter-changes, main, coverage]
name: Check CI status
if: ${{ always() }}
runs-on: ubuntu-latest
steps:
- name: Check CI status
run: |
if [[ "${{ needs.filter-changes.outputs.source_changed }}" == "false" ]]; then
echo "Documentation-only change - CI skipped successfully"
exit 0
fi
if [[ "${{ needs.main.result }}" == "success" && "${{ needs.coverage.result }}" == "success" ]]; then
echo "CI passed"
exit 0
fi
echo "CI failed"
exit 1

View file

@ -2,7 +2,8 @@ name: dockerhub-publish-latest-dagmc-libmesh
on:
push:
branches: master
branches:
- master
jobs:
main:
@ -10,20 +11,20 @@ jobs:
steps:
-
name: Set up QEMU
uses: docker/setup-qemu-action@v2
uses: docker/setup-qemu-action@v3
-
name: Set up Docker Buildx
uses: docker/setup-buildx-action@v2
uses: docker/setup-buildx-action@v3
-
name: Login to DockerHub
uses: docker/login-action@v2
uses: docker/login-action@v3
with:
username: ${{ secrets.DOCKERHUB_USERNAME }}
password: ${{ secrets.DOCKERHUB_TOKEN }}
-
name: Build and push
id: docker_build
uses: docker/build-push-action@v4
uses: docker/build-push-action@v5
with:
push: true
tags: openmc/openmc:latest-dagmc-libmesh

View file

@ -2,7 +2,8 @@ name: dockerhub-publish-latest-dagmc
on:
push:
branches: master
branches:
- master
jobs:
main:
@ -10,20 +11,20 @@ jobs:
steps:
-
name: Set up QEMU
uses: docker/setup-qemu-action@v2
uses: docker/setup-qemu-action@v3
-
name: Set up Docker Buildx
uses: docker/setup-buildx-action@v2
uses: docker/setup-buildx-action@v3
-
name: Login to DockerHub
uses: docker/login-action@v2
uses: docker/login-action@v3
with:
username: ${{ secrets.DOCKERHUB_USERNAME }}
password: ${{ secrets.DOCKERHUB_TOKEN }}
-
name: Build and push
id: docker_build
uses: docker/build-push-action@v4
uses: docker/build-push-action@v5
with:
push: true
tags: openmc/openmc:latest-dagmc

View file

@ -2,7 +2,8 @@ name: dockerhub-publish-develop
on:
push:
branches: develop
branches:
- develop
jobs:
main:
@ -10,20 +11,20 @@ jobs:
steps:
-
name: Set up QEMU
uses: docker/setup-qemu-action@v2
uses: docker/setup-qemu-action@v3
-
name: Set up Docker Buildx
uses: docker/setup-buildx-action@v2
uses: docker/setup-buildx-action@v3
-
name: Login to DockerHub
uses: docker/login-action@v2
uses: docker/login-action@v3
with:
username: ${{ secrets.DOCKERHUB_USERNAME }}
password: ${{ secrets.DOCKERHUB_TOKEN }}
-
name: Build and push
id: docker_build
uses: docker/build-push-action@v4
uses: docker/build-push-action@v5
with:
push: true
tags: openmc/openmc:develop

View file

@ -2,7 +2,8 @@ name: dockerhub-publish-develop-dagmc-libmesh
on:
push:
branches: develop
branches:
- develop
jobs:
main:
@ -10,20 +11,20 @@ jobs:
steps:
-
name: Set up QEMU
uses: docker/setup-qemu-action@v2
uses: docker/setup-qemu-action@v3
-
name: Set up Docker Buildx
uses: docker/setup-buildx-action@v2
uses: docker/setup-buildx-action@v3
-
name: Login to DockerHub
uses: docker/login-action@v2
uses: docker/login-action@v3
with:
username: ${{ secrets.DOCKERHUB_USERNAME }}
password: ${{ secrets.DOCKERHUB_TOKEN }}
-
name: Build and push
id: docker_build
uses: docker/build-push-action@v4
uses: docker/build-push-action@v5
with:
push: true
tags: openmc/openmc:develop-dagmc-libmesh

View file

@ -2,7 +2,8 @@ name: dockerhub-publish-develop-dagmc
on:
push:
branches: develop
branches:
- develop
jobs:
main:
@ -10,20 +11,20 @@ jobs:
steps:
-
name: Set up QEMU
uses: docker/setup-qemu-action@v2
uses: docker/setup-qemu-action@v3
-
name: Set up Docker Buildx
uses: docker/setup-buildx-action@v2
uses: docker/setup-buildx-action@v3
-
name: Login to DockerHub
uses: docker/login-action@v2
uses: docker/login-action@v3
with:
username: ${{ secrets.DOCKERHUB_USERNAME }}
password: ${{ secrets.DOCKERHUB_TOKEN }}
-
name: Build and push
id: docker_build
uses: docker/build-push-action@v4
uses: docker/build-push-action@v5
with:
push: true
tags: openmc/openmc:develop-dagmc

View file

@ -2,7 +2,8 @@ name: dockerhub-publish-develop-libmesh
on:
push:
branches: develop
branches:
- develop
jobs:
main:
@ -10,20 +11,20 @@ jobs:
steps:
-
name: Set up QEMU
uses: docker/setup-qemu-action@v2
uses: docker/setup-qemu-action@v3
-
name: Set up Docker Buildx
uses: docker/setup-buildx-action@v2
uses: docker/setup-buildx-action@v3
-
name: Login to DockerHub
uses: docker/login-action@v2
uses: docker/login-action@v3
with:
username: ${{ secrets.DOCKERHUB_USERNAME }}
password: ${{ secrets.DOCKERHUB_TOKEN }}
-
name: Build and push
id: docker_build
uses: docker/build-push-action@v4
uses: docker/build-push-action@v5
with:
push: true
tags: openmc/openmc:develop-libmesh

View file

@ -2,7 +2,8 @@ name: dockerhub-publish-latest-libmesh
on:
push:
branches: master
branches:
- master
jobs:
main:
@ -10,20 +11,20 @@ jobs:
steps:
-
name: Set up QEMU
uses: docker/setup-qemu-action@v2
uses: docker/setup-qemu-action@v3
-
name: Set up Docker Buildx
uses: docker/setup-buildx-action@v2
uses: docker/setup-buildx-action@v3
-
name: Login to DockerHub
uses: docker/login-action@v2
uses: docker/login-action@v3
with:
username: ${{ secrets.DOCKERHUB_USERNAME }}
password: ${{ secrets.DOCKERHUB_TOKEN }}
-
name: Build and push
id: docker_build
uses: docker/build-push-action@v4
uses: docker/build-push-action@v5
with:
push: true
tags: openmc/openmc:latest-libmesh

View file

@ -2,31 +2,32 @@ name: dockerhub-publish-release-dagmc-libmesh
on:
push:
tags: 'v*.*.*'
tags:
- 'v*.*.*'
jobs:
main:
runs-on: ubuntu-latest
steps:
- uses: actions/checkout@v3
- uses: actions/checkout@v6
- name: Set env
run: echo "RELEASE_VERSION=${GITHUB_REF#refs/*/}" >> $GITHUB_ENV
-
name: Set up QEMU
uses: docker/setup-qemu-action@v2
uses: docker/setup-qemu-action@v3
-
name: Set up Docker Buildx
uses: docker/setup-buildx-action@v2
uses: docker/setup-buildx-action@v3
-
name: Login to DockerHub
uses: docker/login-action@v2
uses: docker/login-action@v3
with:
username: ${{ secrets.DOCKERHUB_USERNAME }}
password: ${{ secrets.DOCKERHUB_TOKEN }}
-
name: Build and push
id: docker_build
uses: docker/build-push-action@v4
uses: docker/build-push-action@v5
with:
push: true
tags: openmc/openmc:${{ env.RELEASE_VERSION }}-dagmc-libmesh

View file

@ -2,31 +2,32 @@ name: dockerhub-publish-release-dagmc
on:
push:
tags: 'v*.*.*'
tags:
- 'v*.*.*'
jobs:
main:
runs-on: ubuntu-latest
steps:
- uses: actions/checkout@v3
- uses: actions/checkout@v6
- name: Set env
run: echo "RELEASE_VERSION=${GITHUB_REF#refs/*/}" >> $GITHUB_ENV
-
name: Set up QEMU
uses: docker/setup-qemu-action@v2
uses: docker/setup-qemu-action@v3
-
name: Set up Docker Buildx
uses: docker/setup-buildx-action@v2
uses: docker/setup-buildx-action@v3
-
name: Login to DockerHub
uses: docker/login-action@v2
uses: docker/login-action@v3
with:
username: ${{ secrets.DOCKERHUB_USERNAME }}
password: ${{ secrets.DOCKERHUB_TOKEN }}
-
name: Build and push
id: docker_build
uses: docker/build-push-action@v4
uses: docker/build-push-action@v5
with:
push: true
tags: openmc/openmc:${{ env.RELEASE_VERSION }}-dagmc

View file

@ -2,31 +2,32 @@ name: dockerhub-publish-release-libmesh
on:
push:
tags: 'v*.*.*'
tags:
- 'v*.*.*'
jobs:
main:
runs-on: ubuntu-latest
steps:
- uses: actions/checkout@v3
- uses: actions/checkout@v6
- name: Set env
run: echo "RELEASE_VERSION=${GITHUB_REF#refs/*/}" >> $GITHUB_ENV
-
name: Set up QEMU
uses: docker/setup-qemu-action@v2
uses: docker/setup-qemu-action@v3
-
name: Set up Docker Buildx
uses: docker/setup-buildx-action@v2
uses: docker/setup-buildx-action@v3
-
name: Login to DockerHub
uses: docker/login-action@v2
uses: docker/login-action@v3
with:
username: ${{ secrets.DOCKERHUB_USERNAME }}
password: ${{ secrets.DOCKERHUB_TOKEN }}
-
name: Build and push
id: docker_build
uses: docker/build-push-action@v4
uses: docker/build-push-action@v5
with:
push: true
tags: openmc/openmc:${{ env.RELEASE_VERSION }}-libmesh

View file

@ -2,31 +2,32 @@ name: dockerhub-publish-release
on:
push:
tags: 'v*.*.*'
tags:
- 'v*.*.*'
jobs:
main:
runs-on: ubuntu-latest
steps:
- uses: actions/checkout@v3
- uses: actions/checkout@v6
- name: Set env
run: echo "RELEASE_VERSION=${GITHUB_REF#refs/*/}" >> $GITHUB_ENV
-
name: Set up QEMU
uses: docker/setup-qemu-action@v2
uses: docker/setup-qemu-action@v3
-
name: Set up Docker Buildx
uses: docker/setup-buildx-action@v2
uses: docker/setup-buildx-action@v3
-
name: Login to DockerHub
uses: docker/login-action@v2
uses: docker/login-action@v3
with:
username: ${{ secrets.DOCKERHUB_USERNAME }}
password: ${{ secrets.DOCKERHUB_TOKEN }}
-
name: Build and push
id: docker_build
uses: docker/build-push-action@v4
uses: docker/build-push-action@v5
with:
push: true
tags: openmc/openmc:${{ env.RELEASE_VERSION }}

View file

@ -2,7 +2,8 @@ name: dockerhub-publish-latest
on:
push:
branches: master
branches:
- master
jobs:
main:
@ -10,20 +11,20 @@ jobs:
steps:
-
name: Set up QEMU
uses: docker/setup-qemu-action@v2
uses: docker/setup-qemu-action@v3
-
name: Set up Docker Buildx
uses: docker/setup-buildx-action@v2
uses: docker/setup-buildx-action@v3
-
name: Login to DockerHub
uses: docker/login-action@v2
uses: docker/login-action@v3
with:
username: ${{ secrets.DOCKERHUB_USERNAME }}
password: ${{ secrets.DOCKERHUB_TOKEN }}
-
name: Build and push
id: docker_build
uses: docker/build-push-action@v4
uses: docker/build-push-action@v5
with:
push: true
tags: openmc/openmc:latest

View file

@ -1,12 +1,28 @@
name: C++ Format Check
on: pull_request
on:
# allow workflow to be run manually
workflow_dispatch:
pull_request:
types:
- opened
- synchronize
- reopened
- labeled
- unlabeled
branches:
- develop
- master
jobs:
cpp-linter:
runs-on: ubuntu-latest
permissions:
contents: read
pull-requests: write
steps:
- uses: actions/checkout@v3
- uses: actions/checkout@v6
- uses: cpp-linter/cpp-linter-action@v2
id: linter
env:
@ -15,11 +31,30 @@ jobs:
style: file
files-changed-only: true
tidy-checks: '-*'
version: '15' # clang-format version
version: '18' # clang-format version
format-review: ${{ github.event_name == 'pull_request' && contains(github.event.pull_request.labels.*.name, 'cpp-format-suggest') }}
passive-reviews: ${{ github.event_name == 'pull_request' && contains(github.event.pull_request.labels.*.name, 'cpp-format-suggest') }}
file-annotations: true
step-summary: true
extensions: 'cpp,h'
- name: Comment with suggestion instructions
if: steps.linter.outputs.checks-failed > 0 && !contains(github.event.pull_request.labels.*.name, 'cpp-format-suggest')
uses: actions/github-script@v7
with:
script: |
const {owner, repo} = context.repo;
const issue_number = context.payload.pull_request.number;
await github.rest.issues.createComment({
owner,
repo,
issue_number,
body: "C++ formatting checks failed. Add the `cpp-format-suggest` label to this PR for inline formatting suggestions on the next run."
});
- name: Failure Check
if: steps.linter.outputs.checks-failed > 0
run: echo "Some files failed the formatting check! See job summary and file annotations for more info" && exit 1
run: |
echo "Some files failed the formatting check."
echo "See job summary and file annotations for details."
exit 1

6
.gitignore vendored
View file

@ -25,12 +25,13 @@ examples/**/*.xml
# Documentation builds
docs/build
docs/doxygen/xml
docs/source/_images/*.pdf
docs/source/_images/*.aux
docs/source/pythonapi/generated/
# Source build
build
build*/
# build from src/utils/setup.py
src/utils/build
@ -104,5 +105,8 @@ CMakeSettings.json
# Visual Studio Code configuration files
.vscode/
# Claude Code agent tools (cached/generated artifacts)
.claude/cache/
# Python pickle files
*.pkl

9
.gitmodules vendored
View file

@ -1,15 +1,6 @@
[submodule "vendor/pugixml"]
path = vendor/pugixml
url = https://github.com/zeux/pugixml.git
[submodule "vendor/gsl-lite"]
path = vendor/gsl-lite
url = https://github.com/martinmoene/gsl-lite.git
[submodule "vendor/xtensor"]
path = vendor/xtensor
url = https://github.com/xtensor-stack/xtensor.git
[submodule "vendor/xtl"]
path = vendor/xtl
url = https://github.com/xtensor-stack/xtl.git
[submodule "vendor/fmt"]
path = vendor/fmt
url = https://github.com/fmtlib/fmt.git

9
.mcp.json Normal file
View file

@ -0,0 +1,9 @@
{
"mcpServers": {
"openmc-code-tools": {
"type": "stdio",
"command": "bash",
"args": [".claude/tools/start_server.sh"]
}
}
}

View file

@ -1,13 +1,23 @@
version: 2
build:
os: "ubuntu-20.04"
os: "ubuntu-24.04"
tools:
python: "3.9"
python: "3.12"
jobs:
post_checkout:
- git fetch --unshallow || true
- cd docs/doxygen && doxygen && cd -
sphinx:
configuration: docs/source/conf.py
formats:
- pdf
python:
install:
- requirements: docs/requirements-rtd.txt
- method: pip
path: .
extra_requirements:
- docs

348
AGENTS.md Normal file
View file

@ -0,0 +1,348 @@
# OpenMC AI Coding Agent Instructions
## Project Overview
OpenMC is a Monte Carlo particle transport code for simulating nuclear reactors,
fusion devices, or other systems with neutron/photon radiation. It's a hybrid
C++17/Python codebase where:
- **C++ core** (`src/`, `include/openmc/`) handles the computationally intensive transport simulation
- **Python API** (`openmc/`) provides user-facing model building, post-processing, and depletion capabilities
- **C API bindings** (`openmc/lib/`) wrap the C++ library via ctypes for runtime control
## Architecture & Key Components
### C++ Component Structure
- **Global vectors of unique_ptrs**: Core objects like `model::cells`, `model::universes`, `nuclides` are stored as `vector<unique_ptr<T>>` in nested namespaces (`openmc::model`, `openmc::simulation`, `openmc::settings`, `openmc::data`)
- **Custom container types**: OpenMC provides its own `vector`, `array`, `unique_ptr`, and `make_unique` in the `openmc::` namespace (defined in `vector.h`, `array.h`, `memory.h`). These are currently typedefs to `std::` equivalents but may become custom implementations for accelerator support. Always use `openmc::vector`, not `std::vector`.
- **Geometry systems**:
- **CSG (default)**: Arbitrarily complex Constructive Solid Geometry using `Surface`, `Region`, `Cell`, `Universe`, `Lattice`
- **DAGMC**: CAD-based geometry via Direct Accelerated Geometry Monte Carlo (optional, requires `OPENMC_USE_DAGMC`)
- **Unstructured mesh**: libMesh-based geometry (optional, requires `OPENMC_USE_LIBMESH`)
- **Particle tracking**: `Particle` class with `GeometryState` manages particle transport through geometry
- **Tallies**: Score quantities during simulation via `Filter` and `Tally` objects
- **Random ray solver**: Alternative deterministic method in `src/random_ray/`
- **Optional features**: DAGMC (CAD geometry), libMesh (unstructured mesh), MPI, all controlled by `#ifdef OPENMC_MPI`, etc.
### Python Component Structure
- **ID management**: All geometry objects (Cell, Surface, Material, etc.) inherit from `IDManagerMixin` which auto-assigns unique integer IDs and tracks them via class-level `used_ids` and `next_id`
- **Input validation**: Extensive use of `openmc.checkvalue` module functions (`check_type`, `check_value`, `check_length`) for all setters
- **XML I/O**: Most classes implement `to_xml_element()` and `from_xml_element()` for serialization to OpenMC's XML input format
- **HDF5 output**: Post-simulation data in statepoint files read via `openmc.StatePoint`
- **Depletion**: `openmc.deplete` implements burnup via operator-splitting with various integrators (Predictor, CECM, etc.)
- **Nuclear Data**: `openmc.data` provides programmatic access to nuclear data files (ENDF, ACE, HDF5)
## Git Branching Workflow
OpenMC uses a git flow branching model with two primary branches:
- **`develop` branch**: The main development branch where all ongoing development takes place. This is the **primary branch against which pull requests are submitted and merged**. This branch is not guaranteed to be stable and may contain work-in-progress features.
- **`master` branch**: The stable release branch containing the latest stable release of OpenMC. This branch only receives merges from `develop` when the development team decides a release should occur.
### Instructions for Code Review
When reviewing code changes in this repository, use the `reviewing-openmc-code` skill.
## Codebase Navigation Tools
Two MCP tools are registered in `.mcp.json` at the repo root and appear
automatically in any MCP-capable agent session.
**`openmc_rag_search`** — Semantic search across the codebase (C++, Python, RST
docs). Finds code by meaning, not just text match. Surfaces related code across
subsystems even when naming differs (e.g., "particle RNG seeding" finds code
across transport, restart, and random ray modes — files you would never find
with `grep "particle seed"`). The index uses a small 22M-param embedding model
(384-dim). Phrase-level natural-language queries work much better than single
keywords or symbol names.
**`openmc_rag_rebuild`** — Rebuild the RAG vector index. Call after pulling new
code or switching branches. The first RAG search of each session will report
the index status and ask whether to rebuild — you can also call this explicitly.
### Why RAG matters
OpenMC is large enough that changes in one subsystem can silently break
invariants that distant subsystems depend on — and those distant files often
use different naming, so grep won't find them. The RAG search finds code by
meaning, surfacing files you wouldn't have thought to open.
An agent reviewed a large OpenMC PR without RAG. It found 1 of 11 serious
bugs. Its post-mortem:
> **I treated the diff as a closed system.** I verified internal consistency of
> the changed code obsessively, but never built a global understanding of how
> the changed code fits into the wider codebase. The diff altered assumptions
> that code elsewhere silently relied on — but I couldn't see that because I
> never looked beyond the diff. I couldn't see the forest for the trees.
>
> **Why I resisted RAG:** Overconfidence. My internal model was "I can see the
> diff, I understand the data structures, I can trace the logic." The diff felt
> self-contained. RAG felt like it would return noisy results about tangentially
> related code. But in a codebase this large, changes in one subsystem can
> quietly break invariants that distant subsystems depend on — and you need
> global awareness to foresee that.
>
> **In the post-mortem**, I re-ran the RAG queries I should have run during the
> review. They directly surfaced the files containing the bugs I missed — files
> I never thought to open because they weren't in the diff.
The takeaway: when reviewing or modifying code, ask yourself "what else in this
codebase might depend on the behavior I'm changing?" If you aren't sure, that's
a good time for a RAG query. It won't replace the grep-based investigation you
should already be doing — but it can surface files you wouldn't have thought to
open.
### Workflow for contributors
1. Create a feature/bugfix branch off `develop`
2. Make changes and commit to the feature branch
3. Open a pull request to merge the feature branch into `develop`
4. A committer reviews and merges the PR into `develop`
## Critical Build & Test Workflows
### Build Dependencies
- **C++17 compiler**: GCC, Clang, or Intel
- **CMake** (3.16+): Required for configuring and building the C++ library
- **HDF5**: Required for cross section data and output file formats
- **libpng**: Used for generating visualization when OpenMC is run in plotting mode
Without CMake and HDF5, OpenMC cannot be compiled.
### Building the C++ Library
```bash
# Configure with CMake (from build/ directory)
cmake .. -DOPENMC_USE_MPI=ON -DOPENMC_USE_OPENMP=ON -DCMAKE_BUILD_TYPE=RelWithDebInfo
# Available CMake options (all default OFF except OPENMC_USE_OPENMP and OPENMC_BUILD_TESTS):
# -DOPENMC_USE_OPENMP=ON/OFF # OpenMP parallelism
# -DOPENMC_USE_MPI=ON/OFF # MPI support
# -DOPENMC_USE_DAGMC=ON/OFF # CAD geometry support
# -DOPENMC_USE_LIBMESH=ON/OFF # Unstructured mesh
# -DOPENMC_ENABLE_PROFILE=ON/OFF # Profiling flags
# -DOPENMC_ENABLE_COVERAGE=ON/OFF # Coverage analysis
# Build
make -j
# C++ unit tests (uses Catch2)
ctest
```
### Python Development
```bash
# Install in development mode (requires building C++ library first)
pip install -e .
# Python tests (uses pytest)
pytest tests/unit_tests/ # Fast unit tests
pytest tests/regression_tests/ # Full regression suite (requires nuclear data)
```
### Nuclear Data Setup (CRITICAL for Running OpenMC)
Most tests require the NNDC HDF5 nuclear cross-section library.
**Important**: Check if `OPENMC_CROSS_SECTIONS` is already set in the user's
environment before downloading, as many users already have nuclear data
installed. Though do note that if this variable is present that it may point to
different cross section data and that the NNDC data is required for tests to
pass.
**If not already configured, download and setup:**
```bash
# Download NNDC HDF5 cross section library (~800 MB compressed)
wget -q -O - https://anl.box.com/shared/static/teaup95cqv8s9nn56hfn7ku8mmelr95p.xz | tar -C $HOME -xJ
# Set environment variable (add to ~/.bashrc or ~/.zshrc for persistence)
export OPENMC_CROSS_SECTIONS=$HOME/nndc_hdf5/cross_sections.xml
```
**Alternative**: Use the provided download script (checks if data exists before downloading):
```bash
bash tools/ci/download-xs.sh # Downloads both NNDC HDF5 and ENDF/B-VII.1 data
```
Without this data, regression tests will fail with "No cross_sections.xml file
found" errors, or, in the case that alternative cross section data is configured
the tests will execute but will not pass. The `cross_sections.xml` file is an
index listing paths to individual HDF5 nuclear data files for each nuclide.
## Testing Expectations
### Environment Requirements
- **Data**: As described above, OpenMC's test suite requires OpenMC to be configured with NNDC data.
- **OpenMP Settings**: OpenMC's tests may fail is more than two OpenMP threads are used. The environment variable `OMP_NUM_THREADS=2` should be set to avoid sporadic test failures.
- **Executable configuration**: The OpenMC executable should compiled with debug symbols enabled.
### C++ Tests
Located in `tests/cpp_unit_tests/`, use Catch2 framework. Run via `ctest` after building with `-DOPENMC_BUILD_TESTS=ON`.
### Python Unit Tests
Located in `tests/unit_tests/`, these are fast, standalone tests that verify Python API functionality without running full simulations. Use standard pytest patterns:
**Categories**:
- **API validation**: Test object creation, property setters/getters, XML serialization (e.g., `test_material.py`, `test_cell.py`, `test_source.py`)
- **Data processing**: Test nuclear data handling, cross sections, depletion chains (e.g., `test_data_neutron.py`, `test_deplete_chain.py`)
- **Library bindings**: Test `openmc.lib` ctypes interface with `model.init_lib()`/`model.finalize_lib()` (e.g., `test_lib.py`)
- **Geometry operations**: Test bounding boxes, containment, lattice generation (e.g., `test_bounding_box.py`, `test_lattice.py`)
**Common patterns**:
- Use fixtures from `tests/unit_tests/conftest.py` (e.g., `uo2`, `water`, `sphere_model`)
- Test invalid inputs with `pytest.raises(ValueError)` or `pytest.raises(TypeError)`
- Use `run_in_tmpdir` fixture for tests that create files
- Tests with `openmc.lib` require calling `model.init_lib()` in try/finally with `model.finalize_lib()`
**Example**:
```python
def test_material_properties():
m = openmc.Material()
m.add_nuclide('U235', 1.0)
assert 'U235' in m.nuclides
with pytest.raises(TypeError):
m.add_nuclide('H1', '1.0') # Invalid type
```
Unit tests should be fast. For tests requiring simulation output, use regression tests instead.
### Python Regression Tests
Regression tests compare OpenMC output against reference data. **Prefer using existing models from `openmc.examples` or those found in tests/unit_tests/conftest.py** (like `pwr_pin_cell()`, `pwr_assembly()`, `slab_mg()`) rather than building from scratch.
**Test Harness Types** (in `tests/testing_harness.py`):
- **PyAPITestHarness**: Standard harness for Python API tests. Compares `inputs_true.dat` (XML hash) and `results_true.dat` (statepoint k-eff and tally values). Requires `model.xml` generation.
- **HashedPyAPITestHarness**: Like PyAPITestHarness but hashes the results for compact comparison
- **TolerantPyAPITestHarness**: For tests with floating-point non-associativity (e.g., random ray solver with single precision). Uses relative tolerance comparisons.
- **WeightWindowPyAPITestHarness**: Compares weight window bounds from `weight_windows.h5`
- **CollisionTrackTestHarness**: Compares collision track data from `collision_track.h5` against `collision_track_true.h5`
- **TestHarness**: Base harness for XML-based tests (no Python model building)
- **PlotTestHarness**: Compares plot output files (PNG or voxel HDF5)
- **CMFDTestHarness**: Specialized for CMFD acceleration tests
- **ParticleRestartTestHarness**: Tests particle restart functionality
Almost all cases use either `PyAPITestHarness` or `HashedPyAPITestHarness`
**Example Test**:
```python
from openmc.examples import pwr_pin_cell
from tests.testing_harness import PyAPITestHarness
def test_my_feature():
model = pwr_pin_cell()
model.settings.particles = 1000 # Modify to exercise feature
harness = PyAPITestHarness('statepoint.10.h5', model)
harness.main()
```
**Workflow**: Create `test.py` and `__init__.py` in `tests/regression_tests/my_test/`, run `pytest --update` to generate reference files (`inputs_true.dat`, `results_true.dat`, etc.), then verify with `pytest` without `--update`. Test results should be generated with `-DOPENMC_ENABLE_STRICT_FP=on` to ensure reproducibility across platforms and optimization levels.
**Critical**: When modifying OpenMC code, regenerate affected test references with `pytest --update` and commit updated reference files.
### Test Configuration
`pytest.ini` sets: `python_files = test*.py`, `python_classes = NoThanks` (disables class-based test collection).
### Testing Options
For builds of OpenMC with MPI enabled, the `--mpi` flag should be passed to the test suite to ensure that appropriate tests are executed using two MPI processes.
The entire test suite can be executed with OpenMC running in event-based mode (instead of the default history-based mode) by providing the `--event` flag to the `pytest` command.
## Cross-Language Boundaries
The C API (defined in `include/openmc/capi.h`) exposes C++ functionality to Python via ctypes bindings in `openmc/lib/`. Example:
```cpp
// C++ API in capi.h
extern "C" int openmc_run();
// Python binding in openmc/lib/core.py
_dll.openmc_run.restype = c_int
def run():
_dll.openmc_run()
```
When modifying C++ public APIs, update corresponding ctypes signatures in `openmc/lib/*.py`.
## Code Style & Conventions
### C++ Style (enforced by .clang-format)
OpenMC generally tries to follow C++ core guidelines where possible
(https://isocpp.github.io/CppCoreGuidelines/CppCoreGuidelines) and follow
modern C++ practices (e.g. RAII) whenever possible.
- **Naming**:
- Classes: `CamelCase` (e.g., `HexLattice`)
- Functions/methods: `snake_case` (e.g., `get_indices`)
- Variables: `snake_case` with trailing underscore for class members (e.g., `n_particles_`, `energy_`)
- Constants: `UPPER_SNAKE_CASE` (e.g., `SQRT_PI`)
- **Namespaces**: All code in `openmc::` namespace, global state in sub-namespaces
- **Include order**: Related header first, then C/C++ stdlib, third-party libs, local headers
- **Comments**: C++-style (`//`) only, never C-style (`/* */`)
- **Standard**: C++17 features allowed
- **Formatting**: Run `clang-format` (version 18) before committing; install via `tools/dev/install-commit-hooks.sh`
### Python Style
- **PEP8** compliant
- **Docstrings**: numpydoc format for all public functions/methods
- **Type hints**: Use sparingly, primarily for complex signatures
- **Path handling**: Use `pathlib.Path` for filesystem operations, accept `str | os.PathLike` in function arguments
- **Dependencies**: Core dependencies only (numpy, scipy, h5py, pandas, matplotlib, lxml, ipython, uncertainties, endf). Other packages must be optional
- **Python version**: Minimum 3.11 (as of Nov 2025)
### ID Management Pattern (Python)
When creating geometry objects, IDs can be auto-assigned or explicit:
```python
# Auto-assigned ID
cell = openmc.Cell() # Gets next available ID
# Explicit ID
cell = openmc.Cell(id=10) # Warning if ID already used
# Reset all IDs (useful in test fixtures)
openmc.reset_auto_ids()
```
### Input Validation Pattern (Python)
All setters use checkvalue functions:
```python
import openmc.checkvalue as cv
@property
def temperature(self):
return self._temperature
@temperature.setter
def temperature(self, temp):
cv.check_type('temperature', temp, Real)
cv.check_greater_than('temperature', temp, 0.0)
self._temperature = temp
```
### Working with HDF5 Files
C++ uses custom HDF5 wrappers in `src/hdf5_interface.cpp`. Python uses h5py directly. Statepoint format version is `VERSION_STATEPOINT` in `include/openmc/constants.h`.
### Conditional Compilation
Check for optional features:
```cpp
#ifdef OPENMC_MPI
// MPI-specific code
#endif
#ifdef OPENMC_DAGMC
// DAGMC-specific code
#endif
```
## Documentation
- **User docs**: Sphinx documentation in `docs/source/` hosted at https://docs.openmc.org
- **C++ docs**: Doxygen-style comments with `\brief`, `\param` tags
- **Python docs**: numpydoc format docstrings
## Common Pitfalls
1. **Forgetting nuclear data**: Tests fail without `OPENMC_CROSS_SECTIONS` environment variable
2. **ID conflicts**: Python objects with duplicate IDs trigger `IDWarning`, use `reset_auto_ids()` between tests
3. **MPI builds**: Code must work with and without MPI; use `#ifdef OPENMC_MPI` guards
4. **Path handling**: Use `pathlib.Path` in new Python code, not `os.path`
5. **Clang-format version**: CI uses version 18; other versions may produce different formatting

68
CITATION.cff Normal file
View file

@ -0,0 +1,68 @@
cff-version: 1.2.0
message: "If you use this software, please cite it as below."
title: OpenMC
authors:
- family-names: Romano
given-names: Paul K.
orcid: "https://orcid.org/0000-0002-1147-045X"
- family-names: Shriwise
given-names: Patrick C.
orcid: "https://orcid.org/0000-0002-3979-7665"
- family-names: Shimwell
given-names: Jonathan
orcid: "https://orcid.org/0000-0001-6909-0946"
- family-names: Harper
given-names: Sterling
- family-names: Boyd
given-names: Will
- family-names: Nelson
given-names: Adam G.
orcid: "https://orcid.org/0000-0002-3614-0676"
- family-names: Tramm
given-names: John R.
orcid: "https://orcid.org/0000-0002-5397-4402"
- family-names: Ridley
given-names: Gavin
orcid: "https://orcid.org/0000-0003-1635-8042"
- family-names: Johnson
given-names: Andrew
orcid: "https://orcid.org/0000-0003-2125-8775"
- family-names: Peterson
given-names: Ethan E.
orcid: "https://orcid.org/0000-0002-5694-7194"
- family-names: Herman
given-names: Bryan R.
preferred-citation:
authors:
- family-names: Romano
given-names: Paul K.
orcid: "https://orcid.org/0000-0002-1147-045X"
- family-names: Horelik
given-names: Nicholas E.
- family-names: Herman
given-names: Bryan R.
- family-names: Nelson
given-names: Adam G.
orcid: "https://orcid.org/0000-0002-3614-0676"
- family-names: Forget
given-names: Benoit
orcid: "https://orcid.org/0000-0003-1459-7672"
- family-names: Smith
given-names: Kord
contact:
- family-names: Romano
given-names: Paul K.
orcid: "https://orcid.org/0000-0002-1147-045X"
doi: 10.1016/j.anucene.2014.07.048
issn: 0306-4549
volume: 82
journal: Annals of Nuclear Energy
publisher:
name: Elsevier
start: 90
end: 97
year: 2015
month: 8
title: "OpenMC: A state-of-the-art Monte Carlo code for research and development"
type: article
url: "https://doi.org/10.1016/j.anucene.2014.07.048"

14
CLAUDE.md Normal file
View file

@ -0,0 +1,14 @@
## OpenMC Codebase Tools
Read the FULL `AGENTS.md` in this directory before starting work. It contains
project context, coding conventions, and documentation of the RAG search tools
registered in `.mcp.json`.
### Claude Code-specific: first-call behavior
The first `openmc_rag_search` call of each session returns an index status
message instead of search results. When this happens, you MUST use the
`AskUserQuestion` tool to present the rebuild/use-existing choice to the user.
Do not ask conversationally — always use the widget. Do not skip this step even
if the index looks current — the user may have uncommitted changes that warrant
a rebuild.

View file

@ -1,11 +1,18 @@
cmake_minimum_required(VERSION 3.10 FATAL_ERROR)
cmake_minimum_required(VERSION 3.16 FATAL_ERROR)
project(openmc C CXX)
# Set version numbers
set(OPENMC_VERSION_MAJOR 0)
set(OPENMC_VERSION_MINOR 14)
set(OPENMC_VERSION_RELEASE 0)
set(OPENMC_VERSION ${OPENMC_VERSION_MAJOR}.${OPENMC_VERSION_MINOR}.${OPENMC_VERSION_RELEASE})
# Set module path
set(CMAKE_MODULE_PATH ${CMAKE_CURRENT_SOURCE_DIR}/cmake/Modules)
include(GetVersionFromGit)
# Output version information
message(STATUS "OpenMC version: ${OPENMC_VERSION}")
message(STATUS "OpenMC dev state: ${OPENMC_DEV_STATE}")
message(STATUS "OpenMC commit hash: ${OPENMC_COMMIT_HASH}")
message(STATUS "OpenMC commit count: ${OPENMC_COMMIT_COUNT}")
# Generate version.h
configure_file(include/openmc/version.h.in "${CMAKE_BINARY_DIR}/include/openmc/version.h" @ONLY)
# Setup output directories
@ -13,12 +20,9 @@ set(CMAKE_ARCHIVE_OUTPUT_DIRECTORY ${CMAKE_BINARY_DIR}/lib)
set(CMAKE_LIBRARY_OUTPUT_DIRECTORY ${CMAKE_BINARY_DIR}/lib)
set(CMAKE_RUNTIME_OUTPUT_DIRECTORY ${CMAKE_BINARY_DIR}/bin)
# Set module path
set(CMAKE_MODULE_PATH ${CMAKE_CURRENT_SOURCE_DIR}/cmake/Modules)
# Allow user to specify <project>_ROOT variables
if (CMAKE_VERSION VERSION_GREATER_EQUAL 3.12)
cmake_policy(SET CMP0074 NEW)
# Generate compile_commands.json for clangd and other tools
if("${CMAKE_EXPORT_COMPILE_COMMANDS}" STREQUAL "")
set(CMAKE_EXPORT_COMPILE_COMMANDS ON)
endif()
# Enable correct usage of CXX_EXTENSIONS
@ -37,8 +41,20 @@ option(OPENMC_ENABLE_COVERAGE "Compile with coverage analysis flags"
option(OPENMC_USE_DAGMC "Enable support for DAGMC (CAD) geometry" OFF)
option(OPENMC_USE_LIBMESH "Enable support for libMesh unstructured mesh tallies" OFF)
option(OPENMC_USE_MPI "Enable MPI" OFF)
option(OPENMC_USE_MCPL "Enable MCPL" OFF)
option(OPENMC_USE_NCRYSTAL "Enable support for NCrystal scattering" OFF)
option(OPENMC_USE_UWUW "Enable UWUW" OFF)
option(OPENMC_FORCE_VENDORED_LIBS "Explicitly use submodules defined in 'vendor'" OFF)
option(OPENMC_ENABLE_STRICT_FP "Enable strict FP flags to improve test portability" OFF)
message(STATUS "OPENMC_USE_OPENMP ${OPENMC_USE_OPENMP}")
message(STATUS "OPENMC_BUILD_TESTS ${OPENMC_BUILD_TESTS}")
message(STATUS "OPENMC_ENABLE_PROFILE ${OPENMC_ENABLE_PROFILE}")
message(STATUS "OPENMC_ENABLE_COVERAGE ${OPENMC_ENABLE_COVERAGE}")
message(STATUS "OPENMC_USE_DAGMC ${OPENMC_USE_DAGMC}")
message(STATUS "OPENMC_USE_LIBMESH ${OPENMC_USE_LIBMESH}")
message(STATUS "OPENMC_USE_MPI ${OPENMC_USE_MPI}")
message(STATUS "OPENMC_USE_UWUW ${OPENMC_USE_UWUW}")
message(STATUS "OPENMC_FORCE_VENDORED_LIBS ${OPENMC_FORCE_VENDORED_LIBS}")
message(STATUS "OPENMC_ENABLE_STRICT_FP ${OPENMC_ENABLE_STRICT_FP}")
# Warnings for deprecated options
foreach(OLD_OPT IN ITEMS "openmp" "profile" "coverage" "dagmc" "libmesh")
@ -80,6 +96,27 @@ if(NOT CMAKE_BUILD_TYPE)
set(CMAKE_BUILD_TYPE RelWithDebInfo CACHE STRING "Choose the type of build" FORCE)
endif()
#===============================================================================
# When STRICT_FP is enabled, remove NDEBUG from RelWithDebInfo flags so that
# assert() remains active. CMake normally adds -DNDEBUG for both Release and
# RelWithDebInfo, which disables C/C++ assert() statements.
#===============================================================================
if(OPENMC_ENABLE_STRICT_FP)
foreach(FLAG_VAR CMAKE_CXX_FLAGS_RELWITHDEBINFO CMAKE_C_FLAGS_RELWITHDEBINFO)
string(REPLACE "-DNDEBUG" "" ${FLAG_VAR} "${${FLAG_VAR}}")
string(REPLACE "/DNDEBUG" "" ${FLAG_VAR} "${${FLAG_VAR}}")
endforeach()
endif()
#===============================================================================
# OpenMP for shared-memory parallelism (and GPU support some day!)
#===============================================================================
if(OPENMC_USE_OPENMP)
find_package(OpenMP REQUIRED)
endif()
#===============================================================================
# MPI for distributed-memory parallelism
#===============================================================================
@ -101,15 +138,6 @@ macro(find_package_write_status pkg)
endif()
endmacro()
#===============================================================================
# NCrystal Scattering Support
#===============================================================================
if(OPENMC_USE_NCRYSTAL)
find_package(NCrystal REQUIRED)
message(STATUS "Found NCrystal: ${NCrystal_DIR} (version ${NCrystal_VERSION})")
endif()
#===============================================================================
# DAGMC Geometry Support - need DAGMC/MOAB
#===============================================================================
@ -117,10 +145,15 @@ endif()
if(OPENMC_USE_DAGMC)
find_package(DAGMC REQUIRED PATH_SUFFIXES lib/cmake)
if (${DAGMC_VERSION} VERSION_LESS 3.2.0)
message(FATAL_ERROR "Discovered DAGMC Version: ${DAGMC_VERSION}. \
Please update DAGMC to version 3.2.0 or greater.")
message(FATAL_ERROR "Discovered DAGMC Version: ${DAGMC_VERSION}."
"Please update DAGMC to version 3.2.0 or greater.")
endif()
message(STATUS "Found DAGMC: ${DAGMC_DIR} (version ${DAGMC_VERSION})")
# Check if UWUW is needed and available
if(OPENMC_USE_UWUW AND NOT DAGMC_BUILD_UWUW)
message(FATAL_ERROR "UWUW is enabled but DAGMC was not configured with UWUW.")
endif()
endif()
#===============================================================================
@ -155,6 +188,11 @@ if(NOT DEFINED HDF5_PREFER_PARALLEL)
endif()
find_package(HDF5 REQUIRED COMPONENTS C HL)
# Remove HDF5 transitive dependencies that are system libraries
list(FILTER HDF5_LIBRARIES EXCLUDE REGEX ".*lib(pthread|dl|m).*")
message(STATUS "HDF5 Libraries: ${HDF5_LIBRARIES}")
if(HDF5_IS_PARALLEL)
if(NOT OPENMC_USE_MPI)
message(FATAL_ERROR "Parallel HDF5 was detected, but MPI was not enabled.\
@ -171,31 +209,33 @@ if(${HDF5_VERSION} VERSION_GREATER_EQUAL 1.12.0)
list(APPEND cxxflags -DH5Oget_info_by_idx_vers=1 -DH5O_info_t_vers=1)
endif()
#===============================================================================
# MCPL
#===============================================================================
if (OPENMC_USE_MCPL)
find_package(MCPL REQUIRED)
message(STATUS "Found MCPL: ${MCPL_DIR} (found version \"${MCPL_VERSION}\")")
endif()
#===============================================================================
# Set compile/link flags based on which compiler is being used
#===============================================================================
# Skip for Visual Studio which has its own configurations through GUI
if(NOT MSVC)
if(OPENMC_USE_OPENMP)
find_package(OpenMP)
if(OPENMP_FOUND)
# In CMake 3.9+, can use the OpenMP::OpenMP_CXX imported target
list(APPEND cxxflags ${OpenMP_CXX_FLAGS})
list(APPEND ldflags ${OpenMP_CXX_FLAGS})
# When OPENMC_ENABLE_STRICT_FP is enabled, disable compiler optimizations that change
# floating-point results relative to -O0, improving cross-platform and
# cross-optimization-level reproducibility for regression testing:
# -ffp-contract=off Prevents FMA contraction (fused multiply-add changes rounding)
# -fno-builtin Prevents replacing math function calls (pow, exp, log, etc.)
# with builtin versions that may differ from libm
# By default (OFF), the compiler is free to use all optimizations for best
# performance.
if(OPENMC_ENABLE_STRICT_FP)
include(CheckCXXCompilerFlag)
check_cxx_compiler_flag(-ffp-contract=off SUPPORTS_FP_CONTRACT_OFF)
if(SUPPORTS_FP_CONTRACT_OFF)
list(APPEND cxxflags -ffp-contract=off)
endif()
check_cxx_compiler_flag(-fno-builtin SUPPORTS_NO_BUILTIN)
if(SUPPORTS_NO_BUILTIN)
list(APPEND cxxflags -fno-builtin)
endif()
endif()
# Skip for Visual Studio which has its own configurations through GUI
if(NOT MSVC)
set(CMAKE_POSITION_INDEPENDENT_CODE ON)
if(OPENMC_ENABLE_PROFILE)
@ -216,8 +256,6 @@ endif()
#===============================================================================
# Update git submodules as needed
#===============================================================================
find_package(Git)
if(GIT_FOUND AND EXISTS "${CMAKE_CURRENT_SOURCE_DIR}/.git")
option(GIT_SUBMODULE "Check submodules during build" ON)
if(GIT_SUBMODULE)
@ -242,49 +280,30 @@ endif()
# pugixml library
#===============================================================================
find_package_write_status(pugixml)
if (NOT pugixml_FOUND)
if(OPENMC_FORCE_VENDORED_LIBS)
add_subdirectory(vendor/pugixml)
set_target_properties(pugixml PROPERTIES CXX_STANDARD 14 CXX_EXTENSIONS OFF)
else()
find_package_write_status(pugixml)
if (NOT pugixml_FOUND)
add_subdirectory(vendor/pugixml)
set_target_properties(pugixml PROPERTIES CXX_STANDARD 14 CXX_EXTENSIONS OFF)
endif()
endif()
#===============================================================================
# {fmt} library
#===============================================================================
find_package_write_status(fmt)
if (NOT fmt_FOUND)
if(OPENMC_FORCE_VENDORED_LIBS)
set(FMT_INSTALL ON CACHE BOOL "Generate the install target.")
add_subdirectory(vendor/fmt)
endif()
#===============================================================================
# xtensor header-only library
#===============================================================================
# CMake 3.13+ will complain about policy CMP0079 unless it is set explicitly
if (CMAKE_VERSION VERSION_GREATER_EQUAL 3.13)
cmake_policy(SET CMP0079 NEW)
endif()
find_package_write_status(xtensor)
if (NOT xtensor_FOUND)
add_subdirectory(vendor/xtl)
set(xtl_DIR ${CMAKE_CURRENT_BINARY_DIR}/vendor/xtl)
add_subdirectory(vendor/xtensor)
endif()
#===============================================================================
# GSL header-only library
#===============================================================================
find_package_write_status(gsl-lite)
if (NOT gsl-lite_FOUND)
add_subdirectory(vendor/gsl-lite)
# Make sure contract violations throw exceptions
target_compile_definitions(gsl-lite-v1 INTERFACE GSL_THROW_ON_CONTRACT_VIOLATION)
target_compile_definitions(gsl-lite-v1 INTERFACE gsl_CONFIG_ALLOWS_NONSTRICT_SPAN_COMPARISON=1)
else()
find_package_write_status(fmt)
if (NOT fmt_FOUND)
set(FMT_INSTALL ON CACHE BOOL "Generate the install target.")
add_subdirectory(vendor/fmt)
endif()
endif()
#===============================================================================
@ -292,9 +311,13 @@ endif()
#===============================================================================
if(OPENMC_BUILD_TESTS)
find_package_write_status(Catch2)
if (NOT Catch2_FOUND)
if (OPENMC_FORCE_VENDORED_LIBS)
add_subdirectory(vendor/Catch2)
else()
find_package_write_status(Catch2)
if (NOT Catch2_FOUND)
add_subdirectory(vendor/Catch2)
endif()
endif()
endif()
@ -332,11 +355,14 @@ endif()
#===============================================================================
list(APPEND libopenmc_SOURCES
src/atomic_mass.cpp
src/bank.cpp
src/boundary_condition.cpp
src/bremsstrahlung.cpp
src/cell.cpp
src/chain.cpp
src/cmfd_solver.cpp
src/collision_track.cpp
src/cross_sections.cpp
src/dagmc.cpp
src/distribution.cpp
@ -353,6 +379,7 @@ list(APPEND libopenmc_SOURCES
src/geometry.cpp
src/geometry_aux.cpp
src/hdf5_interface.cpp
src/ifp.cpp
src/initialize.cpp
src/lattice.cpp
src/material.cpp
@ -363,11 +390,13 @@ list(APPEND libopenmc_SOURCES
src/mgxs.cpp
src/mgxs_interface.cpp
src/ncrystal_interface.cpp
src/ncrystal_load.cpp
src/nuclide.cpp
src/output.cpp
src/particle.cpp
src/particle_data.cpp
src/particle_restart.cpp
src/particle_type.cpp
src/photon.cpp
src/physics.cpp
src/physics_common.cpp
@ -377,6 +406,13 @@ list(APPEND libopenmc_SOURCES
src/progress_bar.cpp
src/random_dist.cpp
src/random_lcg.cpp
src/random_ray/random_ray_simulation.cpp
src/random_ray/random_ray.cpp
src/random_ray/flat_source_domain.cpp
src/random_ray/linear_source_domain.cpp
src/random_ray/moment_matrix.cpp
src/random_ray/source_region.cpp
src/ray.cpp
src/reaction.cpp
src/reaction_product.cpp
src/scattdata.cpp
@ -406,16 +442,24 @@ list(APPEND libopenmc_SOURCES
src/tallies/filter_energyfunc.cpp
src/tallies/filter_legendre.cpp
src/tallies/filter_material.cpp
src/tallies/filter_materialfrom.cpp
src/tallies/filter_mesh.cpp
src/tallies/filter_meshborn.cpp
src/tallies/filter_meshmaterial.cpp
src/tallies/filter_meshsurface.cpp
src/tallies/filter_mu.cpp
src/tallies/filter_musurface.cpp
src/tallies/filter_parent_nuclide.cpp
src/tallies/filter_particle.cpp
src/tallies/filter_particle_production.cpp
src/tallies/filter_polar.cpp
src/tallies/filter_reaction.cpp
src/tallies/filter_sph_harm.cpp
src/tallies/filter_sptl_legendre.cpp
src/tallies/filter_surface.cpp
src/tallies/filter_time.cpp
src/tallies/filter_universe.cpp
src/tallies/filter_weight.cpp
src/tallies/filter_zernike.cpp
src/tallies/tally.cpp
src/tallies/tally_scoring.cpp
@ -476,22 +520,10 @@ if (OPENMC_USE_MPI)
target_compile_definitions(libopenmc PUBLIC -DOPENMC_MPI)
endif()
# Set git SHA1 hash as a compile definition
if(GIT_FOUND)
execute_process(COMMAND ${GIT_EXECUTABLE} rev-parse HEAD
WORKING_DIRECTORY ${CMAKE_CURRENT_SOURCE_DIR}
RESULT_VARIABLE GIT_SHA1_SUCCESS
OUTPUT_VARIABLE GIT_SHA1
ERROR_QUIET OUTPUT_STRIP_TRAILING_WHITESPACE)
if(GIT_SHA1_SUCCESS EQUAL 0)
target_compile_definitions(libopenmc PRIVATE -DGIT_SHA1="${GIT_SHA1}")
endif()
endif()
# target_link_libraries treats any arguments starting with - but not -l as
# linker flags. Thus, we can pass both linker flags and libraries together.
target_link_libraries(libopenmc ${ldflags} ${HDF5_LIBRARIES} ${HDF5_HL_LIBRARIES}
xtensor gsl::gsl-lite-v1 fmt::fmt)
fmt::fmt ${CMAKE_DL_LIBS})
if(TARGET pugixml::pugixml)
target_link_libraries(libopenmc pugixml::pugixml)
@ -500,12 +532,20 @@ else()
endif()
if(OPENMC_USE_DAGMC)
target_compile_definitions(libopenmc PRIVATE DAGMC)
target_link_libraries(libopenmc dagmc-shared uwuw-shared)
target_compile_definitions(libopenmc PUBLIC OPENMC_DAGMC_ENABLED)
target_link_libraries(libopenmc dagmc-shared)
if(OPENMC_USE_UWUW)
target_compile_definitions(libopenmc PRIVATE OPENMC_UWUW_ENABLED)
target_link_libraries(libopenmc uwuw-shared)
endif()
elseif(OPENMC_USE_UWUW)
set(OPENMC_USE_UWUW OFF)
message(FATAL_ERROR "DAGMC must be enabled when UWUW is enabled.")
endif()
if(OPENMC_USE_LIBMESH)
target_compile_definitions(libopenmc PRIVATE LIBMESH)
target_compile_definitions(libopenmc PRIVATE OPENMC_LIBMESH_ENABLED)
target_link_libraries(libopenmc PkgConfig::LIBMESH)
endif()
@ -514,6 +554,10 @@ if (PNG_FOUND)
target_link_libraries(libopenmc PNG::PNG)
endif()
if (OPENMC_USE_OPENMP)
target_link_libraries(libopenmc OpenMP::OpenMP_CXX)
endif()
if (OPENMC_USE_MPI)
target_link_libraries(libopenmc MPI::MPI_CXX)
endif()
@ -524,16 +568,6 @@ if (OPENMC_BUILD_TESTS)
add_subdirectory(tests/cpp_unit_tests)
endif()
if (OPENMC_USE_MCPL)
target_compile_definitions(libopenmc PUBLIC OPENMC_MCPL)
target_link_libraries(libopenmc MCPL::mcpl)
endif()
if(OPENMC_USE_NCRYSTAL)
target_compile_definitions(libopenmc PRIVATE NCRYSTAL)
target_link_libraries(libopenmc NCrystal::NCrystal)
endif()
#===============================================================================
# Log build info that this executable can report later
#===============================================================================
@ -546,6 +580,9 @@ endif()
if (OPENMC_ENABLE_COVERAGE)
target_compile_definitions(libopenmc PRIVATE COVERAGEBUILD)
endif()
if (OPENMC_ENABLE_STRICT_FP)
target_compile_definitions(libopenmc PRIVATE OPENMC_ENABLE_STRICT_FP)
endif()
#===============================================================================
# openmc executable
@ -556,9 +593,9 @@ target_compile_options(openmc PRIVATE ${cxxflags})
target_include_directories(openmc PRIVATE ${CMAKE_BINARY_DIR}/include)
target_link_libraries(openmc libopenmc)
# Ensure C++14 standard is used and turn off GNU extensions
target_compile_features(openmc PUBLIC cxx_std_14)
target_compile_features(libopenmc PUBLIC cxx_std_14)
# Ensure C++17 standard is used and turn off GNU extensions
target_compile_features(openmc PUBLIC cxx_std_17)
target_compile_features(libopenmc PUBLIC cxx_std_17)
set_target_properties(openmc libopenmc PROPERTIES CXX_EXTENSIONS OFF)
#===============================================================================
@ -574,9 +611,7 @@ add_custom_command(TARGET libopenmc POST_BUILD
#===============================================================================
# Install executable, scripts, manpage, license
#===============================================================================
configure_file(cmake/OpenMCConfig.cmake.in "${CMAKE_BINARY_DIR}${CMAKE_FILES_DIRECTORY}/OpenMCConfig.cmake" @ONLY)
configure_file(cmake/OpenMCConfigVersion.cmake.in "${CMAKE_BINARY_DIR}${CMAKE_FILES_DIRECTORY}/OpenMCConfigVersion.cmake" @ONLY)
include(CMakePackageConfigHelpers)
set(INSTALL_CONFIGDIR ${CMAKE_INSTALL_LIBDIR}/cmake/OpenMC)
install(TARGETS openmc libopenmc
@ -590,10 +625,24 @@ install(EXPORT openmc-targets
NAMESPACE OpenMC::
DESTINATION ${INSTALL_CONFIGDIR})
configure_package_config_file(
"cmake/OpenMCConfig.cmake.in"
"${CMAKE_BINARY_DIR}/${CMAKE_FILES_DIRECTORY}/OpenMCConfig.cmake"
INSTALL_DESTINATION ${INSTALL_CONFIGDIR}
)
write_basic_package_version_file(
"${CMAKE_BINARY_DIR}/${CMAKE_FILES_DIRECTORY}/OpenMCConfigVersion.cmake"
VERSION ${OPENMC_VERSION}
COMPATIBILITY AnyNewerVersion
)
install(FILES
"${CMAKE_BINARY_DIR}${CMAKE_FILES_DIRECTORY}/OpenMCConfig.cmake"
"${CMAKE_BINARY_DIR}${CMAKE_FILES_DIRECTORY}/OpenMCConfigVersion.cmake"
DESTINATION ${INSTALL_CONFIGDIR})
"${CMAKE_BINARY_DIR}/${CMAKE_FILES_DIRECTORY}/OpenMCConfig.cmake"
"${CMAKE_BINARY_DIR}/${CMAKE_FILES_DIRECTORY}/OpenMCConfigVersion.cmake"
DESTINATION "${INSTALL_CONFIGDIR}"
)
install(FILES man/man1/openmc.1 DESTINATION ${CMAKE_INSTALL_MANDIR}/man1)
install(FILES LICENSE DESTINATION "${CMAKE_INSTALL_DOCDIR}" RENAME copyright)
install(DIRECTORY include/ DESTINATION ${CMAKE_INSTALL_INCLUDEDIR})

View file

@ -5,9 +5,9 @@ openmc/data/ @paulromano
openmc/lib/ @paulromano
# Depletion
openmc/deplete/ @drewejohnson
tests/regression_tests/deplete/ @drewejohnson
tests/unit_tests/test_deplete_*.py @drewejohnson
openmc/deplete/ @paulromano
tests/regression_tests/deplete/ @paulromano
tests/unit_tests/test_deplete_*.py @paulromano
# MG-related functionality
openmc/mgxs_library.py @nelsonag
@ -26,6 +26,12 @@ src/dagmc.cpp @pshriwise
tests/regression_tests/dagmc/ @pshriwise
tests/unit_tests/dagmc/ @pshriwise
# Weight windows
openmc/weight_windows.py @pshriwise
openmc/lib/weight_windows.py @pshriwise
src/weight_windows.py @pshriwise
tests/unit_tests/weightwindows/ @pshriwise
# Photon transport
openmc/data/BREMX.DAT @amandalund
openmc/data/compton_profiles.h5 @amandalund
@ -49,3 +55,13 @@ openmc/data/resonance_covariance.py @icmeyer
# Docker
Dockerfile @shimwell
# Random ray
src/random_ray/ @jtramm
# NCrystal interface
src/ncrystal_interface.cpp @marquezj @tkittel
src/ncrystal_load.cpp @marquezj @tkittel
# MCPL interface
src/mcpl_interface.cpp @ebknudsen

View file

@ -13,7 +13,7 @@ openmc@anl.gov.
## Resources
- [GitHub Repository](https://github.com/openmc-dev/openmc)
- [Documentation](http://docs.openmc.org/en/latest)
- [Documentation](https://docs.openmc.org/en/latest)
- [Discussion Forum](https://openmc.discourse.group)
- [Slack Community](https://openmc.slack.com/signup) (If you don't see your
domain listed, contact openmc@anl.gov)

View file

@ -24,7 +24,7 @@ ARG compile_cores=1
ARG build_dagmc=off
ARG build_libmesh=off
FROM debian:bullseye-slim AS dependencies
FROM ubuntu:24.04 AS dependencies
ARG compile_cores
ARG build_dagmc
@ -33,22 +33,17 @@ ARG build_libmesh
# Set default value of HOME to /root
ENV HOME=/root
# Embree variables
ENV EMBREE_TAG='v3.12.2'
ENV EMBREE_REPO='https://github.com/embree/embree'
ENV EMBREE_INSTALL_DIR=$HOME/EMBREE/
# MOAB variables
ENV MOAB_TAG='5.3.0'
ENV MOAB_TAG='5.5.1'
ENV MOAB_REPO='https://bitbucket.org/fathomteam/moab/'
# Double-Down variables
ENV DD_TAG='v1.0.0'
ENV DD_TAG='v1.1.0'
ENV DD_REPO='https://github.com/pshriwise/double-down'
ENV DD_INSTALL_DIR=$HOME/Double_down
# DAGMC variables
ENV DAGMC_BRANCH='v3.2.1'
ENV DAGMC_BRANCH='v3.2.4'
ENV DAGMC_REPO='https://github.com/svalinn/DAGMC'
ENV DAGMC_INSTALL_DIR=$HOME/DAGMC/
@ -58,10 +53,11 @@ ENV LIBMESH_REPO='https://github.com/libMesh/libmesh'
ENV LIBMESH_INSTALL_DIR=$HOME/LIBMESH
# NJOY variables
ENV NJOY_TAG='2016.78'
ENV NJOY_REPO='https://github.com/njoy/NJOY2016'
# Setup environment variables for Docker image
ENV LD_LIBRARY_PATH=${DAGMC_INSTALL_DIR}/lib:$LD_LIBRARY_PATH \
ENV LD_LIBRARY_PATH=${DAGMC_INSTALL_DIR}/lib:${LD_LIBRARY_PATH:-} \
OPENMC_ENDF_DATA=/root/endf-b-vii.1 \
DEBIAN_FRONTEND=noninteractive
@ -71,15 +67,19 @@ RUN apt-get update -y && \
apt-get install -y \
python3-pip python-is-python3 wget git build-essential cmake \
mpich libmpich-dev libhdf5-serial-dev libhdf5-mpich-dev \
libpng-dev && \
libpng-dev libpugixml-dev libfmt-dev catch2 python3-venv && \
apt-get autoremove
# create virtual enviroment to avoid externally managed environment error
RUN python3 -m venv openmc_venv
ENV PATH=/openmc_venv/bin:$PATH
# Update system-provided pip
RUN pip install --upgrade pip
# Clone and install NJOY2016
RUN cd $HOME \
&& git clone --single-branch --depth 1 ${NJOY_REPO} \
&& git clone --single-branch -b ${NJOY_TAG} --depth 1 ${NJOY_REPO} \
&& cd NJOY2016 \
&& mkdir build \
&& cd build \
@ -90,28 +90,21 @@ RUN cd $HOME \
RUN if [ "$build_dagmc" = "on" ]; then \
# Install addition packages required for DAGMC
apt-get -y install libeigen3-dev libnetcdf-dev libtbb-dev libglfw3-dev \
&& pip install --upgrade numpy "cython<3.0" \
# Clone and install EMBREE
&& mkdir -p $HOME/EMBREE && cd $HOME/EMBREE \
&& git clone --single-branch -b ${EMBREE_TAG} --depth 1 ${EMBREE_REPO} \
&& mkdir build && cd build \
&& cmake ../embree \
-DCMAKE_INSTALL_PREFIX=${EMBREE_INSTALL_DIR} \
-DEMBREE_MAX_ISA=NONE \
-DEMBREE_ISA_SSE42=ON \
-DEMBREE_ISPC_SUPPORT=OFF \
&& make 2>/dev/null -j${compile_cores} install \
&& rm -rf ${EMBREE_INSTALL_DIR}/build ${EMBREE_INSTALL_DIR}/embree ; \
apt-get -y install \
libeigen3-dev libnetcdf-dev libtbb-dev libglfw3-dev libembree-dev \
&& pip install --upgrade numpy \
&& pip install --no-cache-dir setuptools cython \
# Clone and install MOAB
mkdir -p $HOME/MOAB && cd $HOME/MOAB \
&& mkdir -p $HOME/MOAB && cd $HOME/MOAB \
&& git clone --single-branch -b ${MOAB_TAG} --depth 1 ${MOAB_REPO} \
&& mkdir build && cd build \
&& cmake ../moab -DENABLE_HDF5=ON \
&& cmake ../moab -DCMAKE_BUILD_TYPE=Release \
-DENABLE_HDF5=ON \
-DENABLE_NETCDF=ON \
-DBUILD_SHARED_LIBS=OFF \
-DENABLE_FORTRAN=OFF \
-DENABLE_BLASLAPACK=OFF \
-DENABLE_TESTING=OFF \
&& make 2>/dev/null -j${compile_cores} install \
&& cmake ../moab \
-DENABLE_PYMOAB=ON \
@ -127,7 +120,7 @@ RUN if [ "$build_dagmc" = "on" ]; then \
&& mkdir build && cd build \
&& cmake ../double-down -DCMAKE_INSTALL_PREFIX=${DD_INSTALL_DIR} \
-DMOAB_DIR=/usr/local \
-DEMBREE_DIR=${EMBREE_INSTALL_DIR} \
-DEMBREE_DIR=/usr \
&& make 2>/dev/null -j${compile_cores} install \
&& rm -rf ${DD_INSTALL_DIR}/build ${DD_INSTALL_DIR}/double-down ; \
# Clone and install DAGMC
@ -141,6 +134,7 @@ RUN if [ "$build_dagmc" = "on" ]; then \
-DDOUBLE_DOWN_DIR=${DD_INSTALL_DIR} \
-DCMAKE_PREFIX_PATH=${DD_INSTALL_DIR}/lib \
-DBUILD_STATIC_LIBS=OFF \
-DBUILD_TESTS=OFF \
&& make 2>/dev/null -j${compile_cores} install \
&& rm -rf ${DAGMC_INSTALL_DIR}/DAGMC ${DAGMC_INSTALL_DIR}/build ; \
fi
@ -189,7 +183,7 @@ ENV LIBMESH_INSTALL_DIR=$HOME/LIBMESH
# clone and install openmc
RUN mkdir -p ${HOME}/OpenMC && cd ${HOME}/OpenMC \
&& git clone --shallow-submodules --recurse-submodules --single-branch -b ${openmc_branch} --depth=1 ${OPENMC_REPO} \
&& git clone --shallow-submodules --recurse-submodules --single-branch -b ${openmc_branch} ${OPENMC_REPO} \
&& mkdir build && cd build ; \
if [ ${build_dagmc} = "on" ] && [ ${build_libmesh} = "on" ]; then \
cmake ../openmc \

View file

@ -1,4 +1,4 @@
Copyright (c) 2011-2023 Massachusetts Institute of Technology, UChicago Argonne
Copyright (c) 2011-2026 Massachusetts Institute of Technology, UChicago Argonne
LLC, and OpenMC contributors
Permission is hereby granted, free of charge, to any person obtaining a copy of

View file

@ -26,8 +26,6 @@ recursive-include include *.h
recursive-include include *.h.in
recursive-include include *.hh
recursive-include man *.1
recursive-include openmc *.pyx
recursive-include openmc *.c
recursive-include src *.cc
recursive-include src *.cpp
recursive-include src *.rnc
@ -45,6 +43,5 @@ recursive-include vendor *.hh
recursive-include vendor *.hpp
recursive-include vendor *.pc.in
recursive-include vendor *.natvis
include vendor/gsl-lite/include/gsl/gsl
prune docs/build
prune docs/source/pythonapi/generated/

View file

@ -14,8 +14,8 @@ if(DEFINED ENV{METHOD})
message(STATUS "Using environment variable METHOD to determine libMesh build: ${LIBMESH_PC_FILE}")
endif()
include(FindPkgConfig)
set(ENV{PKG_CONFIG_PATH} "$ENV{PKG_CONFIG_PATH}:${LIBMESH_PC}")
set(PKG_CONFIG_USE_CMAKE_PREFIX_PATH True)
find_package(PkgConfig REQUIRED)
set(PKG_CONFIG_USE_CMAKE_PREFIX_PATH TRUE)
pkg_check_modules(LIBMESH REQUIRED ${LIBMESH_PC_FILE}>=1.7.0 IMPORTED_TARGET)
pkg_get_variable(LIBMESH_PREFIX ${LIBMESH_PC_FILE} prefix)

View file

@ -0,0 +1,120 @@
# GetVersionFromGit.cmake
# Standalone script to retrieve versioning information from Git or .git_archival.txt.
# Customizable for any project by setting variables before including this file.
# Configurable variables:
# - VERSION_PREFIX: Prefix for version tags (default: "v").
# - VERSION_SUFFIX: Suffix for version tags (default: "[~+-]([a-zA-Z0-9]+)").
# - VERSION_REGEX: Regex to extract version (default: "(?[0-9]+\\.[0-9]+\\.[0-9]+)").
# - ARCHIVAL_FILE: Path to .git_archival.txt (default: "${CMAKE_SOURCE_DIR}/.git_archival.txt").
# - DESCRIBE_NAME_KEY: Key for describe name in .git_archival.txt (default: "describe-name: ").
# - COMMIT_HASH_KEY: Key for commit hash in .git_archival.txt (default: "commit: ").
# Default Format Example:
# 1.2.3 v1.2.3 v1.2.3-rc1
set(VERSION_PREFIX "v" CACHE STRING "Prefix used in version tags")
set(VERSION_SUFFIX "[~+-]([a-zA-Z0-9]+)" CACHE STRING "Suffix used in version tags")
set(VERSION_REGEX "?([0-9]+\\.[0-9]+\\.[0-9]+)" CACHE STRING "Regex for extracting version")
set(ARCHIVAL_FILE "${CMAKE_SOURCE_DIR}/.git_archival.txt" CACHE STRING "Path to .git_archival.txt")
set(DESCRIBE_NAME_KEY "describe-name: " CACHE STRING "Key for describe name in .git_archival.txt")
set(COMMIT_HASH_KEY "commit: " CACHE STRING "Key for commit hash in .git_archival.txt")
# Combine prefix and regex
set(VERSION_REGEX_WITH_PREFIX "^${VERSION_PREFIX}${VERSION_REGEX}")
# Find Git
find_package(Git)
# Attempt to retrieve version from Git
if(EXISTS "${CMAKE_SOURCE_DIR}/.git" AND GIT_FOUND)
message(STATUS "Using git describe for versioning")
# Extract the version string
execute_process(
COMMAND git describe --tags --dirty
WORKING_DIRECTORY ${CMAKE_SOURCE_DIR}
OUTPUT_VARIABLE VERSION_STRING
OUTPUT_STRIP_TRAILING_WHITESPACE
ERROR_QUIET
)
# If no tags are found, set version to 0 and show a warning
if(VERSION_STRING STREQUAL "")
set(VERSION_STRING "0.0.0")
message(WARNING
"No git tags found. Version set to 0.0.0.\n"
"Run 'git fetch --tags' to ensure proper versioning.\n"
"For more information, see OpenMC developer documentation."
)
endif()
# Extract the commit hash
execute_process(
COMMAND git rev-parse HEAD
WORKING_DIRECTORY ${CMAKE_SOURCE_DIR}
OUTPUT_VARIABLE COMMIT_HASH
OUTPUT_STRIP_TRAILING_WHITESPACE
)
else()
message(STATUS "Using archival file for versioning: ${ARCHIVAL_FILE}")
if(EXISTS "${ARCHIVAL_FILE}")
file(READ "${ARCHIVAL_FILE}" ARCHIVAL_CONTENT)
# Extract the describe-name line
string(REGEX MATCH "${DESCRIBE_NAME_KEY}([^\\n]+)" VERSION_STRING "${ARCHIVAL_CONTENT}")
if(VERSION_STRING MATCHES "${DESCRIBE_NAME_KEY}(.*)")
set(VERSION_STRING "${CMAKE_MATCH_1}")
else()
message(FATAL_ERROR "Could not extract version from ${ARCHIVAL_FILE}")
endif()
# Extract the commit hash
string(REGEX MATCH "${COMMIT_HASH_KEY}([a-f0-9]+)" COMMIT_HASH "${ARCHIVAL_CONTENT}")
if(COMMIT_HASH MATCHES "${COMMIT_HASH_KEY}([a-f0-9]+)")
set(COMMIT_HASH "${CMAKE_MATCH_1}")
else()
message(FATAL_ERROR "Could not extract commit hash from ${ARCHIVAL_FILE}")
endif()
else()
message(FATAL_ERROR "Neither git describe nor ${ARCHIVAL_FILE} is available for versioning.")
endif()
endif()
# Ensure version string format
if(VERSION_STRING MATCHES "${VERSION_REGEX_WITH_PREFIX}")
set(VERSION_NO_SUFFIX "${CMAKE_MATCH_1}")
else()
message(FATAL_ERROR "Invalid version format: Missing base version in ${VERSION_STRING}")
endif()
# Check for development state
if(VERSION_STRING MATCHES "-([0-9]+)-g([0-9a-f]+)")
set(DEV_STATE "true")
set(COMMIT_COUNT "${CMAKE_MATCH_1}")
string(REGEX REPLACE "-([0-9]+)-g([0-9a-f]+)" "" VERSION_WITHOUT_META "${VERSION_STRING}")
else()
set(DEV_STATE "false")
set(VERSION_WITHOUT_META "${VERSION_STRING}")
endif()
# Split and set version components
string(REPLACE "." ";" VERSION_LIST "${VERSION_NO_SUFFIX}")
list(GET VERSION_LIST 0 VERSION_MAJOR)
list(GET VERSION_LIST 1 VERSION_MINOR)
list(GET VERSION_LIST 2 VERSION_PATCH)
# Increment patch number for dev versions
if(DEV_STATE)
math(EXPR VERSION_PATCH "${VERSION_PATCH} + 1")
endif()
# Export variables
set(OPENMC_VERSION_MAJOR "${VERSION_MAJOR}")
set(OPENMC_VERSION_MINOR "${VERSION_MINOR}")
set(OPENMC_VERSION_PATCH "${VERSION_PATCH}")
set(OPENMC_VERSION "${VERSION_MAJOR}.${VERSION_MINOR}.${VERSION_PATCH}")
set(OPENMC_COMMIT_HASH "${COMMIT_HASH}")
set(OPENMC_DEV_STATE "${DEV_STATE}")
set(OPENMC_COMMIT_COUNT "${COMMIT_COUNT}")

View file

@ -1,17 +1,18 @@
get_filename_component(OpenMC_CMAKE_DIR "${CMAKE_CURRENT_LIST_FILE}" DIRECTORY)
@PACKAGE_INIT@
find_package(fmt REQUIRED HINTS ${OpenMC_CMAKE_DIR}/../fmt)
find_package(gsl-lite REQUIRED HINTS ${OpenMC_CMAKE_DIR}/../gsl-lite)
find_package(pugixml REQUIRED HINTS ${OpenMC_CMAKE_DIR}/../pugixml)
find_package(xtl REQUIRED HINTS ${OpenMC_CMAKE_DIR}/../xtl)
find_package(xtensor REQUIRED HINTS ${OpenMC_CMAKE_DIR}/../xtensor)
if(@OPENMC_USE_DAGMC@)
find_package(DAGMC REQUIRED HINTS @DAGMC_DIR@)
include("${CMAKE_CURRENT_LIST_DIR}/OpenMCConfigVersion.cmake")
include(CMakeFindDependencyMacro)
# Explicitly calculate prefix if it was not generated above
if(NOT DEFINED PACKAGE_PREFIX_DIR)
get_filename_component(PACKAGE_PREFIX_DIR "${CMAKE_CURRENT_LIST_DIR}/../../.." ABSOLUTE)
endif()
if(@OPENMC_USE_NCRYSTAL@)
find_package(NCrystal REQUIRED)
message(STATUS "Found NCrystal: ${NCrystal_DIR} (version ${NCrystal_VERSION})")
find_dependency(fmt CONFIG REQUIRED HINTS ${PACKAGE_PREFIX_DIR})
find_dependency(pugixml CONFIG REQUIRED HINTS ${PACKAGE_PREFIX_DIR})
if(@OPENMC_USE_DAGMC@)
find_dependency(DAGMC REQUIRED HINTS @DAGMC_DIR@)
endif()
if(@OPENMC_USE_LIBMESH@)
@ -21,16 +22,24 @@ if(@OPENMC_USE_LIBMESH@)
pkg_check_modules(LIBMESH REQUIRED @LIBMESH_PC_FILE@>=1.7.0 IMPORTED_TARGET)
endif()
find_package(PNG)
if(NOT TARGET OpenMC::libopenmc)
include("${OpenMC_CMAKE_DIR}/OpenMCTargets.cmake")
if("@PNG_FOUND@")
find_dependency(PNG)
endif()
if(@OPENMC_USE_MPI@)
find_package(MPI REQUIRED)
find_dependency(MPI REQUIRED)
endif()
if(@OPENMC_USE_MCPL@)
find_package(MCPL REQUIRED)
if(@OPENMC_USE_OPENMP@)
find_dependency(OpenMP REQUIRED)
endif()
if(@OPENMC_USE_UWUW@ AND NOT ${DAGMC_BUILD_UWUW})
message(FATAL_ERROR "UWUW is enabled in OpenMC but the DAGMC installation discovered was not configured with UWUW.")
endif()
include("${CMAKE_CURRENT_LIST_DIR}/OpenMCTargets.cmake")
if(NOT OpenMC_FIND_QUIETLY)
message(STATUS "Found OpenMC: ${PACKAGE_VERSION} (found in ${PACKAGE_PREFIX_DIR})")
endif()

View file

@ -1,11 +0,0 @@
set(PACKAGE_VERSION "@OPENMC_VERSION@")
# Check whether the requested PACKAGE_FIND_VERSION is compatible
if("${PACKAGE_VERSION}" VERSION_LESS "${PACKAGE_FIND_VERSION}")
set(PACKAGE_VERSION_COMPATIBLE FALSE)
else()
set(PACKAGE_VERSION_COMPATIBLE TRUE)
if ("${PACKAGE_VERSION}" VERSION_EQUAL "${PACKAGE_FIND_VERSION}")
set(PACKAGE_VERSION_EXACT TRUE)
endif()
endif()

View file

@ -45,6 +45,7 @@ help:
clean:
-rm -rf $(BUILDDIR)/*
-rm -rf source/pythonapi/generated/
-rm -rf doxygen/xml
html:
$(SPHINXBUILD) -b html $(ALLSPHINXOPTS) $(BUILDDIR)/html

13
docs/doxygen/Doxyfile Normal file
View file

@ -0,0 +1,13 @@
# Doxyfile 1.9.1
# This file describes the settings to be used by the documentation system
# doxygen (www.doxygen.org) for a project.
# Difference with default Doxyfile 1.9.1
PROJECT_NAME = OpenMC
QUIET = YES
WARN_IF_UNDOCUMENTED = NO
INPUT = ../../include/openmc/capi.h
GENERATE_HTML = NO
GENERATE_LATEX = NO
GENERATE_XML = YES

View file

@ -1,13 +0,0 @@
sphinx==5.0.2
sphinx_rtd_theme==1.0.0
sphinx-numfig
jupyter
sphinxcontrib-katex
sphinxcontrib-svg2pdfconverter
numpy
scipy
h5py
pandas
uncertainties
matplotlib
lxml

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@ -46,41 +46,29 @@ Type Definitions
Functions
---------
.. c:function:: int openmc_calculate_volumes()
..
Once documentation is complete in capi.h, use:
.. doxygenfile:: capi.h
to populate this documentation without using
.. doxygenfunction::
for every function.
Run a stochastic volume calculation
.. doxygenfunction:: openmc_calculate_volumes
:return: Return status (negative if an error occurred)
:rtype: int
.. doxygenfunction:: openmc_cell_get_fill
.. c:function:: int openmc_cell_get_fill(int32_t index, int* type, int32_t** indices, int32_t* n)
.. doxygenfunction:: openmc_cell_get_id
Get the fill for a cell
.. doxygenfunction:: openmc_cell_get_temperature
.. c:function:: int openmc_cell_get_density(int32_t index, const int32_t* instance, double* density)
Get the density of a cell
:param int32_t index: Index in the cells array
:param int* type: Type of the fill
:param int32_t** indices: Array of material indices for cell
:param int32_t* n: Length of indices array
:return: Return status (negative if an error occurred)
:rtype: int
.. c:function:: int openmc_cell_get_id(int32_t index, int32_t* id)
Get the ID of a cell
:param int32_t index: Index in the cells array
:param int32_t* id: ID of the cell
:return: Return status (negative if an error occurred)
:rtype: int
.. c:function:: int openmc_cell_get_temperature(int32_t index, const int32_t* instance, double* T)
Get the temperature of a cell
:param int32_t index: Index in the cells array
:param int32_t* instance: Which instance of the cell. If a null pointer is passed, the temperature
of the first instance is returned.
:param double* T: temperature of the cell
:param int32_t* instance: Which instance of the cell. If a null pointer is passed, the density
multiplier of the first instance is returned.
:param double* density: Density of the cell in [g/cm3]
:return: Return status (negative if an error occurred)
:rtype: int
@ -113,8 +101,22 @@ Functions
:param double T: Temperature in Kelvin
:param instance: Which instance of the cell. To set the temperature for all
instances, pass a null pointer.
:param set_contained: If the cell is not filled by a material, whether to set the temperatures
of all filled cells
:param bool set_contained: If the cell is not filled by a material, whether
to set the temperatures of all filled cells
:type instance: const int32_t*
:return: Return status (negative if an error occurred)
:rtype: int
.. c:function:: int openmc_cell_set_density(index index, double density, const int32_t* instance, bool set_contained)
Set the density of a cell.
:param int32_t index: Index in the cells array
:param double density: Density of the cell in [g/cm3]
:param instance: Which instance of the cell. To set the density multiplier for all
instances, pass a null pointer.
:param bool set_contained: If the cell is not filled by a material, whether
to set the density multiplier of all filled cells
:type instance: const int32_t*
:return: Return status (negative if an error occurred)
:rtype: int
@ -420,6 +422,16 @@ Functions
:return: Return status (negative if an error occurred)
:rtype: int
.. c:function:: int openmc_mesh_filter_get_mesh(int32_t index, int32_t* index_mesh)
Get the mesh for a mesh filter
:param int32_t index: Index in the filters array
:param index_mesh: Index in the meshes array
:type index_mesh: int32_t*
:return: Return status (negative if an error occurred)
:rtype: int
.. c:function:: int openmc_mesh_filter_set_mesh(int32_t index, int32_t index_mesh)
Set the mesh for a mesh filter
@ -429,6 +441,98 @@ Functions
:return: Return status (negative if an error occurred)
:rtype: int
.. c:function:: int openmc_mesh_filter_get_translation(int32_t index, double translation[3])
Get the 3-D translation coordinates for a mesh filter
:param int32_t index: Index in the filters array
:param double[3] translation: 3-D translation coordinates
:return: Return status (negative if an error occurred)
:rtype: int
.. c:function:: int openmc_mesh_filter_set_translation(int32_t index, double translation[3])
Set the 3-D translation coordinates for a mesh filter
:param int32_t index: Index in the filters array
:param double[3] translation: 3-D translation coordinates
:return: Return status (negative if an error occurred)
:rtype: int
.. c:function:: int openmc_meshborn_filter_get_mesh(int32_t index, int32_t* index_mesh)
Get the mesh for a meshborn filter
:param int32_t index: Index in the filters array
:param index_mesh: Index in the meshes array
:type index_mesh: int32_t*
:return: Return status (negative if an error occurred)
:rtype: int
.. c:function:: int openmc_meshborn_filter_set_mesh(int32_t index, int32_t index_mesh)
Set the mesh for a meshborn filter
:param int32_t index: Index in the filters array
:param int32_t index_mesh: Index in the meshes array
:return: Return status (negative if an error occurred)
:rtype: int
.. c:function:: int openmc_meshborn_filter_get_translation(int32_t index, double translation[3])
Get the 3-D translation coordinates for a meshborn filter
:param int32_t index: Index in the filters array
:param double[3] translation: 3-D translation coordinates
:return: Return status (negative if an error occurred)
:rtype: int
.. c:function:: int openmc_meshborn_filter_set_translation(int32_t index, double translation[3])
Set the 3-D translation coordinates for a meshborn filter
:param int32_t index: Index in the filters array
:param double[3] translation: 3-D translation coordinates
:return: Return status (negative if an error occurred)
:rtype: int
.. c:function:: int openmc_meshsurface_filter_get_mesh(int32_t index, int32_t* index_mesh)
Get the mesh for a mesh surface filter
:param int32_t index: Index in the filters array
:param index_mesh: Index in the meshes array
:type index_mesh: int32_t*
:return: Return status (negative if an error occurred)
:rtype: int
.. c:function:: int openmc_meshsurface_filter_set_mesh(int32_t index, int32_t index_mesh)
Set the mesh for a mesh surface filter
:param int32_t index: Index in the filters array
:param int32_t index_mesh: Index in the meshes array
:return: Return status (negative if an error occurred)
:rtype: int
.. c:function:: int openmc_meshsurface_filter_get_translation(int32_t index, double translation[3])
Get the 3-D translation coordinates for a mesh surface filter
:param int32_t index: Index in the filters array
:param double[3] translation: 3-D translation coordinates
:return: Return status (negative if an error occurred)
:rtype: int
.. c:function:: int openmc_meshsurface_filter_set_translation(int32_t index, double translation[3])
Set the 3-D translation coordinates for a mesh surface filter
:param int32_t index: Index in the filters array
:param double[3] translation: 3-D translation coordinates
:return: Return status (negative if an error occurred)
:rtype: int
.. c:function:: int openmc_next_batch()
Simulate next batch of particles. Must be called after openmc_simulation_init().
@ -453,6 +557,279 @@ Functions
:return: Return status (negative if an error occurs)
:rtype: int
.. c:function:: int openmc_get_plot_index(int32_t id, int32_t* index)
Get the index in the plots array for a plot with a given ID.
:param int32_t id: Plot ID
:param int32_t* index: Index in the plots array
:return: Return status (negative if an error occurred)
:rtype: int
.. c:function:: int openmc_plot_get_id(int32_t index, int32_t* id)
Get the ID of a plot.
:param int32_t index: Index in the plots array
:param int32_t* id: Plot ID
:return: Return status (negative if an error occurred)
:rtype: int
.. c:function:: int openmc_plot_set_id(int32_t index, int32_t id)
Set the ID of a plot.
:param int32_t index: Index in the plots array
:param int32_t id: Plot ID
:return: Return status (negative if an error occurred)
:rtype: int
.. c:function:: size_t openmc_plots_size()
Number of plots currently allocated.
:return: Number of plots in the plots array
:rtype: size_t
.. c:function:: int openmc_solidraytrace_plot_create(int32_t* index)
Create a new solid raytrace plot.
:param int32_t* index: Index of the newly created plot
:return: Return status (negative if an error occurred)
:rtype: int
.. c:function:: int openmc_solidraytrace_plot_get_pixels(int32_t index, int32_t* width, int32_t* height)
Get output pixel dimensions for a solid raytrace plot.
:param int32_t index: Index in the plots array
:param int32_t* width: Image width in pixels
:param int32_t* height: Image height in pixels
:return: Return status (negative if an error occurred)
:rtype: int
.. c:function:: int openmc_solidraytrace_plot_set_pixels(int32_t index, int32_t width, int32_t height)
Set output pixel dimensions for a solid raytrace plot.
:param int32_t index: Index in the plots array
:param int32_t width: Image width in pixels
:param int32_t height: Image height in pixels
:return: Return status (negative if an error occurred)
:rtype: int
.. c:function:: int openmc_solidraytrace_plot_get_color_by(int32_t index, int32_t* color_by)
Get the domain type used for coloring (0=materials, 1=cells).
:param int32_t index: Index in the plots array
:param int32_t* color_by: Coloring mode
:return: Return status (negative if an error occurred)
:rtype: int
.. c:function:: int openmc_solidraytrace_plot_set_color_by(int32_t index, int32_t color_by)
Set the domain type used for coloring (0=materials, 1=cells).
:param int32_t index: Index in the plots array
:param int32_t color_by: Coloring mode
:return: Return status (negative if an error occurred)
:rtype: int
.. c:function:: int openmc_solidraytrace_plot_set_default_colors(int32_t index)
Set default random colors for the current ``color_by`` mode.
:param int32_t index: Index in the plots array
:return: Return status (negative if an error occurred)
:rtype: int
.. c:function:: int openmc_solidraytrace_plot_set_all_opaque(int32_t index)
Mark all domains in the current ``color_by`` mode as opaque.
:param int32_t index: Index in the plots array
:return: Return status (negative if an error occurred)
:rtype: int
.. c:function:: int openmc_solidraytrace_plot_set_opaque(int32_t index, int32_t id, bool visible)
Set whether a specific domain ID is opaque (visible) in the rendered image.
:param int32_t index: Index in the plots array
:param int32_t id: Cell/material ID (based on ``color_by``)
:param bool visible: Whether the domain is opaque
:return: Return status (negative if an error occurred)
:rtype: int
.. c:function:: int openmc_solidraytrace_plot_set_color(int32_t index, int32_t id, uint8_t r, uint8_t g, uint8_t b)
Set RGB color for a specific domain ID.
:param int32_t index: Index in the plots array
:param int32_t id: Cell/material ID (based on ``color_by``)
:param uint8_t r: Red channel
:param uint8_t g: Green channel
:param uint8_t b: Blue channel
:return: Return status (negative if an error occurred)
:rtype: int
.. c:function:: int openmc_solidraytrace_plot_get_color(int32_t index, int32_t id, uint8_t* r, uint8_t* g, uint8_t* b)
Get RGB color for a specific domain ID.
:param int32_t index: Index in the plots array
:param int32_t id: Cell/material ID (based on ``color_by``)
:param uint8_t* r: Red channel
:param uint8_t* g: Green channel
:param uint8_t* b: Blue channel
:return: Return status (negative if an error occurred)
:rtype: int
.. c:function:: int openmc_solidraytrace_plot_get_camera_position(int32_t index, double* x, double* y, double* z)
Get camera position.
:param int32_t index: Index in the plots array
:param double* x: X coordinate
:param double* y: Y coordinate
:param double* z: Z coordinate
:return: Return status (negative if an error occurred)
:rtype: int
.. c:function:: int openmc_solidraytrace_plot_set_camera_position(int32_t index, double x, double y, double z)
Set camera position.
:param int32_t index: Index in the plots array
:param double x: X coordinate
:param double y: Y coordinate
:param double z: Z coordinate
:return: Return status (negative if an error occurred)
:rtype: int
.. c:function:: int openmc_solidraytrace_plot_get_look_at(int32_t index, double* x, double* y, double* z)
Get camera target point.
:param int32_t index: Index in the plots array
:param double* x: X coordinate
:param double* y: Y coordinate
:param double* z: Z coordinate
:return: Return status (negative if an error occurred)
:rtype: int
.. c:function:: int openmc_solidraytrace_plot_set_look_at(int32_t index, double x, double y, double z)
Set camera target point.
:param int32_t index: Index in the plots array
:param double x: X coordinate
:param double y: Y coordinate
:param double z: Z coordinate
:return: Return status (negative if an error occurred)
:rtype: int
.. c:function:: int openmc_solidraytrace_plot_get_up(int32_t index, double* x, double* y, double* z)
Get the camera up vector.
:param int32_t index: Index in the plots array
:param double* x: X component
:param double* y: Y component
:param double* z: Z component
:return: Return status (negative if an error occurred)
:rtype: int
.. c:function:: int openmc_solidraytrace_plot_set_up(int32_t index, double x, double y, double z)
Set the camera up vector.
:param int32_t index: Index in the plots array
:param double x: X component
:param double y: Y component
:param double z: Z component
:return: Return status (negative if an error occurred)
:rtype: int
.. c:function:: int openmc_solidraytrace_plot_get_light_position(int32_t index, double* x, double* y, double* z)
Get light source position.
:param int32_t index: Index in the plots array
:param double* x: X coordinate
:param double* y: Y coordinate
:param double* z: Z coordinate
:return: Return status (negative if an error occurred)
:rtype: int
.. c:function:: int openmc_solidraytrace_plot_set_light_position(int32_t index, double x, double y, double z)
Set light source position.
:param int32_t index: Index in the plots array
:param double x: X coordinate
:param double y: Y coordinate
:param double z: Z coordinate
:return: Return status (negative if an error occurred)
:rtype: int
.. c:function:: int openmc_solidraytrace_plot_get_fov(int32_t index, double* fov)
Get horizontal field of view in degrees.
:param int32_t index: Index in the plots array
:param double* fov: Field of view in degrees
:return: Return status (negative if an error occurred)
:rtype: int
.. c:function:: int openmc_solidraytrace_plot_set_fov(int32_t index, double fov)
Set horizontal field of view in degrees.
:param int32_t index: Index in the plots array
:param double fov: Field of view in degrees
:return: Return status (negative if an error occurred)
:rtype: int
.. c:function:: int openmc_solidraytrace_plot_get_diffuse_fraction(int32_t index, double* diffuse_fraction)
Get diffuse-light fraction.
:param int32_t index: Index in the plots array
:param double* diffuse_fraction: Diffuse fraction in [0, 1]
:return: Return status (negative if an error occurred)
:rtype: int
.. c:function:: int openmc_solidraytrace_plot_set_diffuse_fraction(int32_t index, double diffuse_fraction)
Set diffuse-light fraction.
:param int32_t index: Index in the plots array
:param double diffuse_fraction: Diffuse fraction in [0, 1]
:return: Return status (negative if an error occurred)
:rtype: int
.. c:function:: int openmc_solidraytrace_plot_update_view(int32_t index)
Recompute internal camera/view transforms after camera changes.
:param int32_t index: Index in the plots array
:return: Return status (negative if an error occurred)
:rtype: int
.. c:function:: int openmc_solidraytrace_plot_create_image(int32_t index, uint8_t* data_out, int32_t width, int32_t height)
Render the plot to an RGB image buffer.
:param int32_t index: Index in the plots array
:param uint8_t* data_out: Output buffer of shape ``height*width*3``
:param int32_t width: Image width in pixels
:param int32_t height: Image height in pixels
:return: Return status (negative if an error occurred)
:rtype: int
.. c:function:: int openmc_reset()
Resets all tally scores
@ -474,6 +851,10 @@ Functions
:return: Return status (negative if an error occurs)
:rtype: int
.. c:function:: void openmc_run_random_ray()
Run a random ray simulation
.. c:function:: int openmc_set_n_batches(int32_t n_batches, bool set_max_batches, bool add_statepoint_batch)
Set number of batches and number of max batches

View file

@ -11,7 +11,10 @@
# All configuration values have a default; values that are commented out
# serve to show the default.
import sys, os
import os
from pathlib import Path
import subprocess
import sys
# Determine if we're on Read the Docs server
on_rtd = os.environ.get('READTHEDOCS', None) == 'True'
@ -37,6 +40,7 @@ sys.path.insert(0, os.path.abspath('../..'))
# Add any Sphinx extension module names here, as strings. They can be extensions
# coming with Sphinx (named 'sphinx.ext.*') or your custom ones.
extensions = [
'breathe',
'sphinx.ext.autodoc',
'sphinx.ext.napoleon',
'sphinx.ext.autosummary',
@ -47,12 +51,14 @@ extensions = [
]
if not on_rtd:
extensions.append('sphinxcontrib.rsvgconverter')
doxygen_dir = Path(__file__).parents[1] / 'doxygen'
subprocess.run(['doxygen'], cwd=doxygen_dir, check=True)
# Add any paths that contain templates here, relative to this directory.
templates_path = ['_templates']
# The suffix of source filenames.
source_suffix = '.rst'
source_suffix = {'.rst': 'restructuredtext'}
# The encoding of source files.
#source_encoding = 'utf-8'
@ -62,16 +68,17 @@ master_doc = 'index'
# General information about the project.
project = 'OpenMC'
copyright = '2011-2023, Massachusetts Institute of Technology, UChicago Argonne LLC, and OpenMC contributors'
copyright = '2011-2026, Massachusetts Institute of Technology, UChicago Argonne LLC, and OpenMC contributors'
# The version info for the project you're documenting, acts as replacement for
# |version| and |release|, also used in various other places throughout the
# built documents.
#
# The short X.Y version.
version = "0.14"
import openmc
# The full version, including alpha/beta/rc tags.
release = "0.14.0"
version = release = openmc.__version__
# The language for content autogenerated by Sphinx. Refer to documentation
# for a list of supported languages.
@ -116,13 +123,17 @@ pygments_style = 'tango'
# A list of ignored prefixes for module index sorting.
#modindex_common_prefix = []
# -- Options breathe + doxygen -------------------------------------------------
breathe_projects = {"OpenMC": "../doxygen/xml"}
breathe_default_project = "OpenMC"
breathe_domain_by_file_pattern = {"*capi.h": "c"}
# -- Options for HTML output ---------------------------------------------------
# The theme to use for HTML and HTML Help pages
import sphinx_rtd_theme
html_theme = 'sphinx_rtd_theme'
html_theme_path = [sphinx_rtd_theme.get_html_theme_path()]
html_baseurl = "https://docs.openmc.org/en/stable/"
html_logo = '_images/openmc_logo.png'

View file

@ -0,0 +1,104 @@
.. _devguide_agentic_tools:
===========================
Agentic Development Tools
===========================
OpenMC ships a set of tools designed for AI coding agents (such as
`Claude Code`_) that agents can use to navigate and understand the codebase.
.. _Claude Code: https://claude.ai/code
Motivation
----------
Agentic tools like Claude Code are skilled at using grep to navigate and
understand large code bases. However, grep can only find exact text matches —
it cannot discover code that is *conceptually* related but uses different
naming. Without a "global view" of the codebase that a human developer will
build up over time, the agent is generally blind to any file it hasn't
tokenized fully. While it can grep to see who else calls a function, it
remains blind if other areas might be related but not share identical naming
conventions.
This problem is mitigated somewhat by using a model with a longer context
window. OpenMC has somewhere around ~1 million tokens of C++ and ~1 million
tokens of python. While Claude Code in early 2026 only has a context window
of 200k tokens, beta versions have extended context windows of 1M tokens,
and it's not unreasonable to assume that models may be available in the near
future that greatly exceed these limits.
However, even assuming the entire repository can be fit within a context
window, there are several downsides to doing this.
`Model performance degrades significantly as context size increases`_.
Benchmark results are
greatly improved if the model has less garbage to pick through. Additionally, API usage
is typically billed as tokens in/out per turn. As the context file
grows these costs become much larger. As such, there is still significant
motivation to solving the above problem, so as to ensure only relevant
information is drawn into context so as to maximize model performance and
minimize costs.
Setup
-----
The tools are registered as an `MCP (Model Context Protocol)`_ server in
``.mcp.json`` at the repository root. AI agents that support MCP (such as
Claude Code) discover them automatically on session start. The underlying
Python scripts can also be run directly from the command line.
All tools run entirely locally — no API keys or external service accounts are
required. Python dependencies are installed automatically into an isolated
virtual environment at ``.claude/cache/.venv/`` on first use.
.. _Model performance degrades significantly as context size increases: https://www.anthropic.com/news/claude-opus-4-6
.. _MCP (Model Context Protocol): https://modelcontextprotocol.io
RAG Semantic Search
-------------------
The RAG (Retrieval-Augmented Generation) semantic search addresses this
problem — it finds code by meaning, not just text match, surfacing related code
across subsystems that ``grep`` would miss entirely. Two MCP tools are provided:
- **openmc_rag_search** — Given a natural-language query, returns the most
relevant code chunks with file paths, line numbers, and a preview. Can search
code, documentation, or both. Can also find code related to a given file.
- **openmc_rag_rebuild** — Rebuilds the search index. Should be called after
pulling new code or switching branches.
How it works
^^^^^^^^^^^^
The search pipeline runs entirely on your local CPU:
1. **Chunking.** All C++, Python, and RST files are split into overlapping
fixed-size windows (~1000 characters, 25% overlap). This ensures every line
of code appears in at least one chunk and most lines appear in two.
2. **Embedding.** Each chunk is embedded into a 384-dimensional vector using
the `all-MiniLM-L6-v2`_ sentence-transformer model (22 million parameters).
This model runs on CPU with no GPU required. No API key is needed — the
model weights are downloaded once from Hugging Face and cached locally.
3. **Indexing.** The vectors are stored in a local LanceDB_ database on disk.
Building the full index takes approximately 5 minutes on a machine with
10 CPU cores. The index is stored in ``.claude/cache/rag_index/`` and
persists across sessions.
4. **Searching.** Your query is embedded using the same model, and the closest
chunks are retrieved by vector similarity. Results include the file path,
line range, file type, similarity distance, and a text preview.
.. _all-MiniLM-L6-v2: https://huggingface.co/sentence-transformers/all-MiniLM-L6-v2
.. _LanceDB: https://lancedb.com
Requirements
^^^^^^^^^^^^
No system dependencies beyond **Python 3.12+** with ``pip``. An internet
connection is required on first use to download the Python packages and
embedding model weights; subsequent runs are fully offline. The Python packages
(``sentence-transformers``, ``lancedb``) and their dependencies (including
PyTorch, ~2GB) are installed automatically into an isolated virtual environment
on first use.

View file

@ -109,9 +109,10 @@ Leadership Team
The TC consists of the following individuals:
- `Paul Romano <https://github.com/paulromano>`_
- `Sterling Harper <https://github.com/smharper>`_
- `Patrick Shriwise <https://github.com/pshriwise>`_
- `Adam Nelson <https://github.com/nelsonag>`_
- `Benoit Forget <https://github.com/bforget>`_
- `Jonathan Shimwell <https://github.com/shimwell>`_
- `John Tramm <https://github.com/jtramm>`_
The Project Lead is Paul Romano.

View file

@ -12,7 +12,12 @@ Python API. That is, from the root directory of the OpenMC repository:
.. code-block:: sh
python -m pip install .[docs]
python -m pip install ".[docs]"
The OpenMC documentation also uses Doxygen to automatically generate its
C/C++ API documentation directly from the docstrings available in the source
code. You will need to have a working installation of Doxygen to generate the
documentation locally.
-----------------------------------
Building Documentation as a Webpage

View file

@ -45,12 +45,11 @@ Now you can run the following to create a `Docker container`_ called
This command will open an interactive shell running from within the
Docker container where you have access to use OpenMC.
.. note:: The ``docker run`` command supports many
`options <https://docs.docker.com/engine/reference/commandline/run/>`_
.. note:: The ``docker run`` command supports many options_
for spawning containers -- including `mounting volumes`_ from the
host filesystem -- which many users will find useful.
.. _Docker image: https://docs.docker.com/engine/reference/commandline/images/
.. _Docker image: https://docs.docker.com/get-started/docker-concepts/the-basics/what-is-an-image/
.. _Docker container: https://www.docker.com/resources/what-container
.. _options: https://docs.docker.com/engine/reference/commandline/run/
.. _mounting volumes: https://docs.docker.com/storage/volumes/
.. _options: https://docs.docker.com/reference/cli/docker/container/run/
.. _mounting volumes: https://docs.docker.com/engine/storage/volumes/

View file

@ -14,7 +14,9 @@ other related topics.
contributing
workflow
agentic-tools
styleguide
policies
tests
user-input
docbuild

View file

@ -0,0 +1,35 @@
.. _devguide_policies:
========
Policies
========
---------------------
Python Version Policy
---------------------
OpenMC follows the Scientific Python Ecosystem Coordination guidelines `SPEC 0
<https://scientific-python.org/specs/spec-0000/>`_ on minimum supported
versions, which recommends that support for Python versions be dropped 3 years
after their initial release.
-------------------
C++ Standard Policy
-------------------
C++ code in OpenMC must conform to the most recent C++ standard that is fully
supported in the `version of the gcc compiler
<https://gcc.gnu.org/projects/cxx-status.html>`_ that is distributed with the
oldest version of Ubuntu that is still within its `standard support period
<https://ubuntu.com/about/release-cycle>`_. Ubuntu 22.04 LTS will be supported
through April 2027 and is distributed with gcc 11.4.0, which fully supports the
C++17 standard.
--------------------
CMake Version Policy
--------------------
Similar to the C++ standard policy, the minimum supported version of CMake
corresponds to whatever version is distributed with the oldest version of Ubuntu
still within its standard support period. Ubuntu 22.04 LTS is distributed with
CMake 3.22.

View file

@ -30,7 +30,7 @@ whenever a file is saved. For example, `Visual Studio Code
support for running clang-format.
.. note::
OpenMC's CI uses `clang-format` version 15. A different version of `clang-format`
OpenMC's CI uses `clang-format` version 18. A different version of `clang-format`
may produce different line changes and as a result fail the CI test.
Miscellaneous
@ -40,14 +40,15 @@ Follow the `C++ Core Guidelines`_ except when they conflict with another
guideline listed here. For convenience, many important guidelines from that
list are repeated here.
Conform to the C++14 standard.
Conform to the C++17 standard.
Always use C++-style comments (``//``) as opposed to C-style (``/**/``). (It
is more difficult to comment out a large section of code that uses C-style
comments.)
Do not use C-style casting. Always use the C++-style casts ``static_cast``,
``const_cast``, or ``reinterpret_cast``. (See `ES.49 <http://isocpp.github.io/CppCoreGuidelines/CppCoreGuidelines#es49-if-you-must-use-a-cast-use-a-named-cast>`_)
``const_cast``, or ``reinterpret_cast``. (See `ES.49
<https://isocpp.github.io/CppCoreGuidelines/CppCoreGuidelines#es49-if-you-must-use-a-cast-use-a-named-cast>`_)
Source Files
------------
@ -55,7 +56,7 @@ Source Files
Use a ``.cpp`` suffix for code files and ``.h`` for header files.
Header files should always use include guards with the following style (See
`SF.8 <http://isocpp.github.io/CppCoreGuidelines/CppCoreGuidelines#sf8-use-include-guards-for-all-h-files>`_):
`SF.8 <https://isocpp.github.io/CppCoreGuidelines/CppCoreGuidelines#Rs-guards>`_):
.. code-block:: C++
@ -146,7 +147,7 @@ Style for Python code should follow PEP8_.
Docstrings for functions and methods should follow numpydoc_ style.
Python code should work with Python 3.7+.
Python code should work with Python 3.8+.
Use of third-party Python packages should be limited to numpy_, scipy_,
matplotlib_, pandas_, and h5py_. Use of other third-party packages must be
@ -156,11 +157,11 @@ Prefer pathlib_ when working with filesystem paths over functions in the os_
module or other standard-library modules. Functions that accept arguments that
represent a filesystem path should work with both strings and Path_ objects.
.. _C++ Core Guidelines: http://isocpp.github.io/CppCoreGuidelines/CppCoreGuidelines
.. _PEP8: https://www.python.org/dev/peps/pep-0008/
.. _C++ Core Guidelines: https://isocpp.github.io/CppCoreGuidelines/CppCoreGuidelines
.. _PEP8: https://peps.python.org/pep-0008/
.. _numpydoc: https://numpydoc.readthedocs.io/en/latest/format.html
.. _numpy: https://numpy.org/
.. _scipy: https://www.scipy.org/
.. _scipy: https://scipy.org/
.. _matplotlib: https://matplotlib.org/
.. _pandas: https://pandas.pydata.org/
.. _h5py: https://www.h5py.org/

View file

@ -37,6 +37,9 @@ Prerequisites
- Some tests require `NJOY <https://www.njoy21.io/NJOY2016>`_ to preprocess
cross section data. The test suite assumes that you have an ``njoy``
executable available on your :envvar:`PATH`.
- OpenMC should be compiled with ``-DOPENMC_ENABLE_STRICT_FP=on`` to ensure
reproducible floating-point results across platforms and optimization levels.
Without this flag, regression tests may not match reference values.
Running Tests
-------------
@ -67,9 +70,11 @@ make sure you have satisfied all the prerequisites above. After you have done
that, consider the following:
- When building OpenMC, make sure you run CMake with
``-DCMAKE_BUILD_TYPE=Debug``. Building with a release build will result in
some test failures due to differences in which compiler optimizations are
used.
``-DOPENMC_ENABLE_STRICT_FP=on``. This prevents the compiler from applying
floating-point optimizations (such as replacing math library calls with
builtins or contracting multiply-add into FMA instructions) that can produce
bit-level differences across platforms and optimization levels. Any
``CMAKE_BUILD_TYPE`` can be used.
- Because tallies involve the sum of many floating point numbers, the
non-associativity of floating point numbers can result in different answers
especially when the number of threads is high (different order of operations).
@ -84,6 +89,30 @@ that, consider the following:
limit the number of threads that OpenBLAS uses internally; this can be done by
setting the :envvar:`OPENBLAS_NUM_THREADS` environment variable to 1.
Debugging Tests in CI
---------------------
Tests can be debugged in CI using a feature called
`tmate <https://github.com/mxschmitt/action-tmate?tab=readme-ov-file#debug-your-github-actions-by-using-tmate>`_.
CI debugging can be
enabled by including "[gha-debug]" in the commit message. When the test fails, a
link similar to the one shown below will be provided in the GitHub Actions
output after failure occurs. Logging into the provided link will allow you to
debug the test in the CI environment. The following is an example of the output
shown in the CI log that provides the link to the tmate session:
.. code-block:: text
:linenos:
Created new session successfully
ssh 2VcykjU7vNdvAzEjQcc839GM2@nyc1.tmate.io
https://tmate.io/t/2VcykjU7vNdvAzEjQcc839GM2
Entering main loop
Web shell: https://tmate.io/t/2VcykjU7vNdvAzEjQcc839GM2
SSH: ssh 2VcykjU7vNdvAzEjQcc839GM2@nyc1.tmate.io
...
Generating XML Inputs
---------------------
@ -134,6 +163,12 @@ following files to your new test directory:
compiler options during openmc configuration and build (e.g., no MPI, no
debug/optimization).
For tests using the Python API, both the **inputs_true.dat** and
**results_true.dat** files can be generated automatically in the correct format
via::
pytest --update <name-of-test>
In addition to this description, please see the various types of tests that are
already included in the test suite to see how to create them. If all is
implemented correctly, the new test will automatically be discovered by pytest.

View file

@ -55,6 +55,6 @@ developer or send a message to the `developers mailing list`_.
.. _property attribute: https://docs.python.org/3.6/library/functions.html#property
.. _XML Schema Part 2: http://www.w3.org/TR/xmlschema-2/
.. _boolean: http://www.w3.org/TR/xmlschema-2/#boolean
.. _XML Schema Part 2: https://www.w3.org/TR/xmlschema-2/
.. _boolean: https://www.w3.org/TR/xmlschema-2/#boolean
.. _developers mailing list: https://groups.google.com/forum/?fromgroups=#!forum/openmc-dev

View file

@ -91,6 +91,30 @@ features and bug fixes. The general steps for contributing are as follows:
6. After the pull request has been thoroughly vetted, it is merged back into the
*develop* branch of openmc-dev/openmc.
Setting Up Upstream Tracking (Required for Versioning)
------------------------------------------------------
By default, your fork **does not** include tags from the upstream OpenMC repository.
OpenMC relies on `git describe --tags` for versioning in source builds, and missing tags can lead
to incorrect version detection (i.e., ``0.0.0``). To ensure proper versioning, follow these steps:
1. **Add the Upstream Repository**
This allows you to fetch updates from the main OpenMC repository.
.. code-block:: sh
git remote add upstream https://github.com/openmc-dev/openmc.git
2. **Fetch and Push Tags**
Retrieve tags from the upstream repository and update your fork:
.. code-block:: sh
git fetch --tags upstream
git push --tags origin
This ensures that both your **local** and **remote** fork have the correct versioning information.
Private Development
-------------------
@ -126,10 +150,10 @@ reinstalling it). While the same effect can be achieved using the
:envvar:`PYTHONPATH` environment variable, this is generally discouraged as it
can interfere with virtual environments.
.. _git: http://git-scm.com/
.. _git: https://git-scm.com/
.. _GitHub: https://github.com/
.. _git flow: https://nvie.com/git-model
.. _valgrind: https://www.valgrind.org/
.. _valgrind: https://valgrind.org/
.. _style guide: https://docs.openmc.org/en/latest/devguide/styleguide.html
.. _pull request: https://docs.github.com/en/github/collaborating-with-issues-and-pull-requests/about-pull-requests
.. _openmc-dev/openmc: https://github.com/openmc-dev/openmc

View file

@ -12,7 +12,7 @@ files produced by NJOY. Parallelism is enabled via a hybrid MPI and OpenMP
programming model.
OpenMC was originally developed by members of the `Computational Reactor Physics
Group <http://crpg.mit.edu>`_ at the `Massachusetts Institute of Technology
Group <https://crpg.mit.edu>`_ at the `Massachusetts Institute of Technology
<https://web.mit.edu>`_ starting in 2011. Various universities, laboratories,
and other organizations now contribute to the development of OpenMC. For more
information on OpenMC, feel free to post a message on the `OpenMC Discourse

View file

@ -0,0 +1,46 @@
.. _io_collision_track:
===========================
Collision Track File Format
===========================
When collision tracking is enabled with ``mcpl=false`` (the default), OpenMC
writes binary data to an HDF5 file named ``collision_track.h5``. The same data
may also be written after each batch when multiple files are requested
(``collision_track.N.h5``) or when the run is performed in parallel. The file
contains the information needed to reconstruct each recorded collision.
The current revision of the collision track file format is 1.2.
**/**
:Attributes:
- **filetype** (*char[]*) -- String indicating the type of file.
For collision-track files the value is ``"collision_track"``.
:Datasets:
- **collision_track_bank** (Compound type) -- Collision information
for each stored event. Each entry in the dataset corresponds to one
collision and contains the following fields:
- ``r`` (*double[3]*) -- Position of the collision in [cm].
- ``u`` (*double[3]*) -- Direction unit vector immediately after the collision.
- ``E`` (*double*) -- Incident particle energy before the collision in [eV].
- ``dE`` (*double*) -- Energy loss over the collision (:math:`E_\text{before} - E_\text{after}`) in [eV].
- ``time`` (*double*) -- Time of the collision in [s].
- ``wgt`` (*double*) -- Particle weight at the collision.
- ``event_mt`` (*int*) -- ENDF MT number identifying the reaction.
- ``delayed_group`` (*int*) -- Delayed neutron group index (non-zero for delayed events).
- ``cell_id`` (*int*) -- ID of the cell in which the collision occurred.
- ``nuclide_id`` (*int*) -- PDG number of the nuclide (100ZZZAAAM).
- ``material_id`` (*int*) -- ID of the material containing the collision site.
- ``universe_id`` (*int*) -- ID of the universe containing the collision site.
- ``n_collision`` (*int*) -- Collision counter for the particle history.
- ``particle`` (*int32_t*) -- Particle type (PDG number).
- ``parent_id`` (*int64_t*) -- Unique ID of the parent particle.
- ``progeny_id`` (*int64_t*) -- Progeny ID of the particle.
In an MPI run, OpenMC writes the combined dataset by gathering collision-track
entries from all ranks before flushing them to disk, so the final file appears
as though it were produced serially.

View file

@ -56,6 +56,27 @@ attributes:
.. _io_chain_reaction:
--------------------
``<source>`` Element
--------------------
The ``<source>`` element represents photon and electron sources associated with
the decay of a nuclide and contains information to construct an
:class:`openmc.stats.Univariate` object that represents this emission as an
energy distribution. This element has the following attributes:
:type:
The type of :class:`openmc.stats.Univariate` source term.
:particle:
The type of particle emitted, e.g., 'photon' or 'electron'
:parameters:
The parameters of the source term, e.g., for a
:class:`openmc.stats.Discrete` source, the energies (in [eV]) at which the
particles are emitted and their relative intensities in [Bq/atom] (in other
words, decay constants).
----------------------
``<reaction>`` Element
----------------------

View file

@ -4,7 +4,7 @@
Depletion Results File Format
=============================
The current version of the depletion results file format is 1.1.
The current version of the depletion results file format is 1.3.
**/**
@ -12,30 +12,31 @@ The current version of the depletion results file format is 1.1.
- **version** (*int[2]*) -- Major and minor version of the
statepoint file format.
:Datasets: - **eigenvalues** (*double[][][2]*) -- k-eigenvalues at each
time/stage. This array has shape (number of timesteps, number of
stages, value). The last axis contains the eigenvalue and the
associated uncertainty
- **number** (*double[][][][]*) -- Total number of atoms. This array
has shape (number of timesteps, number of stages, number of
:Datasets: - **eigenvalues** (*double[][2]*) -- k-eigenvalues at each timestep.
This array has shape (number of timesteps, 2). The second axis
contains the eigenvalue and its associated uncertainty.
- **number** (*double[][][]*) -- Total number of atoms at each
timestep. This array has shape (number of timesteps, number of
materials, number of nuclides).
- **reaction rates** (*double[][][][][]*) -- Reaction rates used to
build depletion matrices. This array has shape (number of
timesteps, number of stages, number of materials, number of
nuclides, number of reactions).
- **reaction rates** (*double[][][][]*) -- Reaction rates at each
timestep. This array has shape (number of timesteps, number of
materials, number of nuclides, number of reactions). Only stored if
write_rates=True.
- **time** (*double[][2]*) -- Time in [s] at beginning/end of each
step.
- **source_rate** (*double[][]*) -- Power in [W] or source rate in
[neutron/sec]. This array has shape (number of timesteps, number
of stages).
- **source_rate** (*double[]*) -- Power in [W] or source rate in
[neutron/sec] for each timestep.
- **depletion time** (*double[]*) -- Average process time in [s]
spent depleting a material across all burnable materials and,
if applicable, MPI processes.
- **keff_search_root** (*double[]*) -- Root of the keff search at the
end of the timestep, if applicable.
**/materials/<id>/**
:Attributes: - **index** (*int*) -- Index used in results for this material
- **volume** (*double*) -- Volume of this material in [cm^3]
- **name** (*char[]*) -- Name of this material
**/nuclides/<name>/**

View file

@ -38,11 +38,9 @@ Each ``<surface>`` element can have the following attributes or sub-elements:
:boundary:
The boundary condition for the surface. This can be "transmission",
"vacuum", "reflective", or "periodic". Periodic boundary conditions can
only be applied to x-, y-, and z-planes. Only axis-aligned periodicity is
supported, i.e., x-planes can only be paired with x-planes. Specify which
planes are periodic and the code will automatically identify which planes
are paired together.
"vacuum", "reflective", or "periodic". Specify which planes are
periodic and the code will automatically identify which planes are
paired together.
*Default*: "transmission"
@ -318,9 +316,10 @@ the following attributes or sub-elements:
*Default*: None
:orientation:
The orientation of the hexagonal lattice. The string "x" indicates that two
sides of the lattice are parallel to the x-axis, whereas the string "y"
indicates that two sides are parallel to the y-axis.
The orientation of the hexagonal lattice. The string "x" indicates that each
lattice element has two faces that are perpendicular to the x-axis, whereas
the string "y" indicates that each lattice element has two faces that are
perpendicular to the y-axis.
*Default*: "y"
@ -407,13 +406,64 @@ Each ``<dagmc_universe>`` element can have the following attributes or sub-eleme
*Default*: None
:cell:
Zero or more ``<cell>`` sub-elements may appear to override properties of
individual DAGMC volumes. Each ``<cell>`` element supports the following
attributes and sub-elements:
.. note:: A geometry.xml file containing only a DAGMC model for a file named `dagmc.h5m` (no CSG)
looks as follows
:id:
The integer cell ID in the DAGMC geometry to override. Required.
.. code-block:: xml
:name:
An optional string label for the cell.
<?xml version='1.0' encoding='utf-8'?>
<geometry>
<dagmc_universe filename="dagmc.h5m" id="1" />
</geometry>
*Default*: None
:material:
The material ID to assign to this cell. Use ``void`` for vacuum. Multiple
space-separated IDs may be given to specify a distribmat (distributed
material) assignment. Required.
:temperature:
Temperature(s) in [K] to assign to the cell. Must be greater than or equal
to 0. Multiple space-separated values may be given.
*Default*: None
:density:
Density in [g/cm³] to assign to the cell. Must be greater than 0. Requires a non-void
material fill. Multiple space-separated values may be given.
*Default*: None
:volume:
Volume of the cell in [cm³].
.. note:: DAGMC can compute cell volumes exactly from the triangulated
mesh surfaces. Specifying a manual volume risks inconsistency
with that capability.
*Default*: None
The following standard ``<cell>`` attributes are **not** supported inside
``<dagmc_universe>`` and will raise an error if present: ``region``,
``fill``, ``universe``, ``translation``, ``rotation``.
.. deprecated::
The ``<material_overrides>`` sub-element (containing ``<cell_override>``
children with ``<material_ids>``) is deprecated. A deprecation warning is
emitted and the overrides are converted to the ``<cell>`` format at parse
time. It is an error to specify both ``<material_overrides>`` and
``<cell>`` sub-elements on the same ``<dagmc_universe>``.
*Default*: None
.. note:: A geometry.xml file containing only a DAGMC model for a file named
`dagmc.h5m` (no CSG) looks as follows:
.. code-block:: xml
<?xml version='1.0' encoding='utf-8'?>
<geometry>
<dagmc_universe filename="dagmc.h5m" id="1" />
</geometry>

View file

@ -44,6 +44,7 @@ Output Files
statepoint
source
collision_track
summary
properties
depletion_results

View file

@ -133,6 +133,10 @@ Temperature-dependent data, provided for temperature <TTT>K.
This dataset is optional. This is a 1-D vector if `representation`
is "isotropic", or a 3-D vector if `representation` is "angle"
with dimensions of [polar][azimuthal][groups].
When this data is not available, an approximation using the
group energy boundaries is used. For more information see
the particle speed subsection in the multigroup-data section
of the theory manual.
**/<library name>/<TTT>K/scatter_data/**

View file

@ -4,7 +4,7 @@
Particle Restart File Format
============================
The current version of the particle restart file format is 2.0.
The current version of the particle restart file format is 2.1.
**/**
@ -26,8 +26,7 @@ The current version of the particle restart file format is 2.0.
- **run_mode** (*char[]*) -- Run mode used, either 'fixed source',
'eigenvalue', or 'particle restart'.
- **id** (*int8_t*) -- Unique identifier of the particle.
- **type** (*int*) -- Particle type (0=neutron, 1=photon, 2=electron,
3=positron)
- **type** (*int32_t*) -- Particle type (PDG number)
- **weight** (*double*) -- Weight of the particle.
- **energy** (*double*) -- Energy of the particle in eV for
continuous-energy mode, or the energy group of the particle for

View file

@ -7,13 +7,18 @@ Geometry Plotting Specification -- plots.xml
Basic plotting capabilities are available in OpenMC by creating a plots.xml file
and subsequently running with the ``--plot`` command-line flag. The root element
of the plots.xml is simply ``<plots>`` and any number output plots can be
defined with ``<plot>`` sub-elements. Two plot types are currently implemented
defined with ``<plot>`` sub-elements. Four plot types are currently implemented
in openMC:
* ``slice`` 2D pixel plot along one of the major axes. Produces a PNG image
file.
* ``voxel`` 3D voxel data dump. Produces an HDF5 file containing voxel xyz
position and cell or material id.
* ``wireframe_raytrace`` 2D pixel plot of a three-dimensional view of a
geometry using wireframes around cells or materials and coloring by depth
through each material.
* ``solid_raytrace`` 2D pixel plot of a three-dimensional view of a geometry
with solid colored surfaces of a set of cells or materials.
------------------
@ -66,21 +71,22 @@ sub-elements:
*Default*: None - Required entry
:type:
Keyword for type of plot to be produced. Currently only "slice" and "voxel"
plots are implemented. The "slice" plot type creates 2D pixel maps saved in
the PNG file format. The "voxel" plot type produces a binary datafile
containing voxel grid positioning and the cell or material (specified by the
``color`` tag) at the center of each voxel. Voxel plot files can be
processed into VTK files using the :ref:`scripts_voxel` script provided with
OpenMC and subsequently viewed with a 3D viewer such as VISIT or Paraview.
See the :ref:`io_voxel` for information about the datafile structure.
Keyword for type of plot to be produced. Currently "slice", "voxel",
"wireframe_raytrace", and "solid_raytrace" plots are implemented. The
"slice" plot type creates 2D pixel maps saved in the PNG file format. The
"voxel" plot type produces a binary datafile containing voxel grid
positioning and the cell or material (specified by the ``color`` tag) at the
center of each voxel. Voxel plot files can be processed into VTK files using
the :func:`openmc.voxel_to_vtk` function and subsequently viewed with a 3D
viewer such as VISIT or Paraview. See :ref:`io_voxel` for information about
the datafile structure.
.. note:: High-resolution voxel files produced by OpenMC can be quite large,
but the equivalent VTK files will be significantly smaller.
*Default*: "slice"
``<plot>`` elements of ``type`` "slice" and "voxel" must contain the ``pixels``
All ``<plot>`` elements must contain the ``pixels``
attribute or sub-element:
:pixels:
@ -96,7 +102,7 @@ attribute or sub-element:
``width``/``pixels`` along that basis direction may not appear
in the plot.
*Default*: None - Required entry for "slice" and "voxel" plots
*Default*: None - Required entry for all plots
``<plot>`` elements of ``type`` "slice" can also contain the following
attributes or sub-elements. These are not used in "voxel" plots:
@ -125,6 +131,11 @@ attributes or sub-elements. These are not used in "voxel" plots:
Specifies the custom color for the cell or material. Should be 3 integers
separated by spaces.
:xs:
The attenuation coefficient for volume rendering of color in units of
inverse centimeters. Zero corresponds to transparency. Only for plot type
"wireframe_raytrace".
As an example, if your plot is colored by material and you want material 23
to be blue, the corresponding ``color`` element would look like:
@ -151,6 +162,18 @@ attributes or sub-elements. These are not used in "voxel" plots:
*Default*: 255 255 255 (white)
:show_overlaps:
Indicates whether overlapping regions of different cells are shown.
*Default*: None
:overlap_color:
Specifies the RGB color of overlapping regions of different cells. Does not
do anything if ``show_overlaps`` is "false" or not specified. Should be 3
integers separated by spaces.
*Default*: 255 0 0 (red)
:meshlines:
The ``meshlines`` sub-element allows for plotting the boundaries of a
regular mesh on top of a plot. Only one ``meshlines`` element is allowed per
@ -179,3 +202,80 @@ attributes or sub-elements. These are not used in "voxel" plots:
*Default*: 0 0 0 (black)
*Default*: None
``<plot>`` elements of ``type`` "wireframe_raytrace" or "solid_raytrace" can contain the
following attributes or sub-elements.
:camera_position:
Location in 3D Cartesian space the camera is at.
*Default*: None - Required for all ``wireframe_raytrace`` or
``solid_raytrace`` plots
:look_at:
Location in 3D Cartesian space the camera is looking at.
*Default*: None - Required for all ``wireframe_raytrace`` or
``solid_raytrace`` plots
:field_of_view:
The horizontal field of view in degrees. Defaults to roughly the same value
as for the human eye.
*Default*: 70
:orthographic_width:
If set to a nonzero value, an orthographic rather than perspective
projection for the camera is employed. An orthographic projection puts out
parallel rays from the camera of a width prescribed here in the horizontal
direction, with the width in the vertical direction decided by the pixel
aspect ratio.
*Default*: 0
``<plot>`` elements of ``type`` "solid_raytrace" can contain the following attributes or
sub-elements.
:opaque_ids:
List of integer IDs of cells or materials to be treated as visible in the
plot. Whether the integers are interpreted as cell or material IDs depends
on ``color_by``.
*Default*: None - Required for all phong plots
:light_position:
Location in 3D Cartesian space of the light.
*Default*: Same location as ``camera_position``
:diffuse_fraction:
Fraction of light originating from non-directional sources. If set to one,
the coloring is not influenced by surface curvature, and no shadows appear.
If set to zero, only regions illuminated by the light are not black.
*Default*: 0.1
``<plot>`` elements of ``type`` "wireframe_raytrace" can contain the following
attributes or sub-elements.
:wireframe_color:
RGB value of the wireframe's color
*Default*: 0, 0, 0 (black)
:wireframe_thickness:
Integer number of pixels that the wireframe takes up. The value is a radius
of the wireframe. Setting to zero removes any wireframing.
*Default*: 0
:wireframe_ids:
Integer IDs of cells or materials of regions to draw wireframes around.
Whether the integers are interpreted as cell or material IDs depends on
``color_by``.
*Default*: None

View file

@ -4,7 +4,7 @@
Properties File Format
======================
The current version of the properties file format is 1.0.
The current version of the properties file format is 1.1.
**/**
@ -25,6 +25,7 @@ The current version of the properties file format is 1.0.
**/geometry/cells/cell <uid>/**
:Datasets: - **temperature** (*double[]*) -- Temperature of the cell in [K].
- **density** (*double[]*) -- Density of the cell in [g/cm3].
**/materials/**

View file

@ -7,6 +7,19 @@ Settings Specification -- settings.xml
All simulation parameters and miscellaneous options are specified in the
settings.xml file.
-------------------------------
``<atomic_relaxation>`` Element
-------------------------------
The ``<atomic_relaxation>`` element determines whether the atomic relaxation
cascade, the X-ray fluorescence photons and Auger electrons emitted when an
inner-shell vacancy is filled, is simulated following photoelectric and
incoherent (Compton) scattering interactions. Disabling this can speed up
photon transport calculations where the detailed secondary particle cascade is
not of interest.
*Default*: true
---------------------
``<batches>`` Element
---------------------
@ -20,6 +33,90 @@ source neutrons.
*Default*: None
-----------------------------
``<collision_track>`` Element
-----------------------------
The ``<collision_track>`` element indicates to track information about particle
collisions based on a set of criteria and store these events in a file named
``collision_track.h5``. This file records details such as the position of the
interaction, direction of the incoming particle, incident energy and deposited
energy, weight, time of the interaction, and the delayed neutron group (0 for
prompt neutrons). Additional information such as the cell ID, material ID,
universe ID, nuclide ZAID, particle type, and event MT number are also stored.
Users can specify one or more criterion to filter collisions. If no criteria are
specified, it defaults to tracking all collisions across the model.
.. warning::
Storing all collisions can be very memory intensive. For more targeted
tracking, users can employ a variety of parameters such as ``cell_ids``,
``reactions``, ``universe_ids``, ``material_ids``, ``nuclides``, and
``deposited_E_threshold`` to refine the selection of particle interactions
to be banked.
This element can contain one or more of the following attributes or
sub-elements:
:max_collisions:
An integer indicating the maximum number of collisions to be banked per file.
*Default*: 1000
:max_collision_track_files:
An integer indicating the number of collision_track files to be used.
*Default*: 1
:mcpl:
An optional boolean to enable MCPL_-format instead of the native HDF5-based
format. If activated, the output file name and type is changed to
``collision_track.mcpl``.
*Default*: false
.. _MCPL: https://mctools.github.io/mcpl/mcpl.pdf
:cell_ids:
A list of integers representing cell IDs to define specific cells in which
collisions are to be banked.
*Default*: None
:universe_ids:
A list of integers representing the universe IDs to define specific
universes in which collisions are to be banked.
*Default*: None
:material_ids:
A list of integers representing the material IDs to define specific
materials in which collisions are to be banked.
*Default*: None
:nuclides:
A list of strings representing the nuclide, to define specific
define specific target nuclide collisions to be banked.
.. note::
Electron and positron collision-track events are not associated with
a specific nuclide. If a ``nuclides`` entry is specified, these events
are omitted.
*Default*: None
:reactions:
A list of integers representing the ENDF-6 format MT numbers or strings
(e.g. (n,fission)) to define specific reaction types to be banked.
*Default*: None
:deposited_E_threshold:
A float defining the minimum deposited energy per collision (in eV) to
trigger banking.
*Default*: 0.0
----------------------------------
``<confidence_intervals>`` Element
----------------------------------
@ -81,6 +178,13 @@ time.
*Default*: 1.0
:survival_normalization:
If this element is set to "true", this will enable the use of survival
biasing source normalization, whereby the weight parameters, weight and
weight_avg, are multiplied per history by the start weight of said history.
*Default*: false
:energy_neutron:
The energy under which neutrons will be killed.
@ -171,6 +275,16 @@ history-based parallelism.
*Default*: false
--------------------------------
``<free_gas_threshold>`` Element
--------------------------------
The ``<free_gas_threshold>`` element specifies the energy multiplier, expressed
in units of :math:`kT`, that determines when the free gas scattering approach is
used for elastic scattering. Values must be positive.
*Default*: 400.0
-----------------------------------
``<generations_per_batch>`` Element
-----------------------------------
@ -181,6 +295,15 @@ ignored for all run modes other than "eigenvalue".
*Default*: 1
------------------------------
``<ifp_n_generation>`` Element
------------------------------
The ``<ifp_n_generation>`` element indicates the number of generations to
consider for the Iterated Fission Probability method.
*Default*: 10
----------------------
``<inactive>`` Element
----------------------
@ -238,7 +361,7 @@ based on the recommended value in LA-UR-14-24530_.
.. note:: This element is not used in the multi-group :ref:`energy_mode`.
.. _LA-UR-14-24530: https://laws.lanl.gov/vhosts/mcnp.lanl.gov/pdf_files/la-ur-14-24530.pdf
.. _LA-UR-14-24530: https://mcnp.lanl.gov/pdf_files/TechReport_2014_LANL_LA-UR-14-24530_Brown.pdf
---------------------------
``<material_cell_offsets>``
@ -252,19 +375,45 @@ to false.
*Default*: true
----------------------------------------
``<max_particles_in_flight>`` Element
----------------------------------------
--------------------------------
``<max_lost_particles>`` Element
--------------------------------
This element indicates the number of neutrons to run in flight concurrently
This element indicates the maximum number of lost particles.
*Default*: 10
------------------------------------
``<rel_max_lost_particles>`` Element
------------------------------------
This element indicates the maximum number of lost particles, relative to the
total number of particles.
*Default*: 1.0e-6
-------------------------------------
``<max_particles_in_flight>`` Element
-------------------------------------
This element indicates the number of particles to run in flight concurrently
when using event-based parallelism. A higher value uses more memory, but
may be more efficient computationally.
*Default*: 100000
---------------------------
---------------------------------
``<max_particle_events>`` Element
---------------------------------
This element indicates the maximum number of events a particle can undergo.
*Default*: 1000000
-----------------------
``<max_order>`` Element
---------------------------
-----------------------
The ``<max_order>`` element allows the user to set a maximum scattering order
to apply to every nuclide/material in the problem. That is, if the data
@ -276,6 +425,31 @@ then, OpenMC will only use up to the :math:`P_1` data.
.. note:: This element is not used in the continuous-energy
:ref:`energy_mode`.
--------------------------------
``<max_history_splits>`` Element
--------------------------------
The ``<max_history_splits>`` element indicates the number of times a particle
can split during a history.
*Default*: 1000
-----------------------------
``<max_secondaries>`` Element
-----------------------------
The ``<max_secondaries>`` element indicates the maximum secondary bank size.
*Default*: 10000
------------------------
``<max_tracks>`` Element
------------------------
The ``<max_tracks>`` element indicates the maximum number of tracks written to a
track file (per MPI process).
*Default*: 1000
--------------------------------------
``<max_write_lost_particles>`` Element
@ -386,6 +560,18 @@ generator during generation of colors in plots.
*Default*: 1
.. _properties_file:
-----------------------------
``<properties_file>`` Element
-----------------------------
The ``properties_file`` element has no attributes and contains the path to a
properties HDF5 file to load cell temperatures/densities and material
densities.
*Default*: None
---------------------
``<ptables>`` Element
---------------------
@ -398,6 +584,93 @@ or sub-elements and can be set to either "false" or "true".
.. note:: This element is not used in the multi-group :ref:`energy_mode`.
------------------------
``<random_ray>`` Element
------------------------
The ``<random_ray>`` element enables random ray mode and contains a number of
settings relevant to the solver. Tips for selecting these parameters can be
found in the :ref:`random ray user guide <random_ray>`.
:distance_inactive:
The inactive ray length (dead zone length) in [cm].
*Default*: None
:distance_active:
The active ray length in [cm].
*Default*: None
:ray_source:
Specifies the starting ray distribution, and follows the format for
:ref:`source_element`. It must be uniform in space and angle and cover the
full domain. It does not represent a physical neutron or photon source -- it
is only used to sample integrating ray starting locations and directions.
*Default*: None
:adjoint_source:
Specifies an adjoint fixed source for adjoint transport simulations, and
follows the format for :ref:`source_element`. The distributions which make
up the adjoint source are subject to the same restrictions as forward
fixed sources in Random Ray mode.
*Default*: None
:adjoint:
Specifies whether to perform adjoint transport. The default is 'False',
corresponding to forward transport.
*Default*: None
:volume_estimator:
Specifies choice of volume estimator for the random ray solver. Options
are 'naive', 'simulation_averaged', or 'hybrid'. The default is 'hybrid'.
*Default*: None
:volume_normalized_flux_tallies:
Specifies whether to normalize flux tallies by volume (bool). The
default is 'False'. When enabled, flux tallies will be reported in units
of cm/cm^3. When disabled, flux tallies will be reported in units of cm
(i.e., total distance traveled by neutrons in the spatial tally
region).
*Default*: None
:sample_method:
Specifies the method for sampling the starting ray distribution. This
element can be set to "prng" or "halton".
*Default*: prng
:source_region_meshes:
Relates meshes to spatial domains for subdividing source regions with each domain.
:mesh:
Contains an ``id`` attribute and one or more ``<domain>`` sub-elements.
:id:
The unique identifier for the mesh.
:domain:
Each domain element has an ``id`` attribute and a ``type`` attribute.
:id:
The unique identifier for the domain.
:type:
The type of the domain. Can be ``material``, ``cell``, or ``universe``.
:diagonal_stabilization_rho:
The rho factor for use with diagonal stabilization. This technique is
applied when negative diagonal (in-group) elements are detected in
the scattering matrix of input MGXS data, which is a common feature
of transport corrected MGXS data.
*Default*: 1.0
----------------------------------
``<resonance_scattering>`` Element
----------------------------------
@ -473,6 +746,19 @@ pseudo-random number generator.
*Default*: 1
-----------------------------------
``<shared_secondary_bank>`` Element
-----------------------------------
The ``shared_secondary_bank`` element indicates whether to use a shared
secondary particle bank. When enabled, secondary particles are collected into
a global bank, sorted for reproducibility, and load-balanced across MPI ranks
between generations. If not specified, the shared secondary bank is enabled
automatically for fixed-source simulations with weight windows active, and
disabled otherwise.
.. _source_element:
--------------------
``<source>`` Element
--------------------
@ -491,10 +777,15 @@ attributes/sub-elements:
*Default*: 1.0
:type:
Indicator of source type. One of ``independent``, ``file``, or ``compiled``.
Indicator of source type. One of ``independent``, ``file``, ``compiled``,
``mesh``, or ``tokamak``. The type of the source will be determined by this
attribute if it is present.
:particle:
The source particle type, either ``neutron`` or ``photon``.
The source particle type, specified as a PDG number or a string alias (e.g.,
``neutron``/``n``, ``photon``/``gamma``, ``electron``, ``positron``,
``proton``/``p``, ``deuteron``/``d``, ``triton``/``t``, ``alpha``, or GNDS
nuclide names like ``Fe57``).
*Default*: neutron
@ -534,24 +825,38 @@ attributes/sub-elements:
:type:
The type of spatial distribution. Valid options are "box", "fission",
"point", "cartesian", "cylindrical", and "spherical". A "box" spatial
distribution has coordinates sampled uniformly in a parallelepiped. A
"fission" spatial distribution samples locations from a "box"
"point", "cartesian", "cylindrical", "spherical", "mesh", and "cloud".
A "box" spatial distribution has coordinates sampled uniformly in a
parallelepiped.
A "fission" spatial distribution samples locations from a "box"
distribution but only locations in fissionable materials are accepted.
A "point" spatial distribution has coordinates specified by a triplet.
A "cartesian" spatial distribution specifies independent distributions of
x-, y-, and z-coordinates. A "cylindrical" spatial distribution specifies
independent distributions of r-, phi-, and z-coordinates where phi is the
azimuthal angle and the origin for the cylindrical coordinate system is
specified by origin. A "spherical" spatial distribution specifies
independent distributions of r-, cos_theta-, and phi-coordinates where
cos_theta is the cosine of the angle with respect to the z-axis, phi is
the azimuthal angle, and the sphere is centered on the coordinate
(x0,y0,z0). A "mesh" spatial distribution samples source sites from a mesh element
x-, y-, and z-coordinates.
A "cylindrical" spatial distribution specifies independent distributions
of r-, phi-, and z-coordinates where phi is the azimuthal angle and the
origin for the cylindrical coordinate system is specified by origin.
A "spherical" spatial distribution specifies independent distributions of
r-, cos_theta-, and phi-coordinates where cos_theta is the cosine of the
angle with respect to the z-axis, phi is the azimuthal angle, and the
sphere is centered on the coordinate (x0,y0,z0).
A "mesh" spatial distribution samples source sites from a mesh element
based on the relative strengths provided in the node. Source locations
within an element are sampled isotropically. If no strengths are provided,
the space within the mesh is uniformly sampled.
A "cloud" spatial distribution samples source sites from a list of spatial
positions provided in the node, based on the relative strengths provided
in the node. If no strengths are provided, the positions are uniformly
sampled.
*Default*: None
:parameters:
@ -570,6 +875,7 @@ attributes/sub-elements:
For a "cylindrical" distribution, no parameters are specified. Instead,
the ``r``, ``phi``, ``z``, and ``origin`` elements must be specified.
Optionally, the ``r_dir`` and ``z_dir`` elements could be specified.
For a "spherical" distribution, no parameters are specified. Instead,
the ``r``, ``theta``, ``phi``, and ``origin`` elements must be specified.
@ -601,6 +907,10 @@ attributes/sub-elements:
of a univariate probability distribution (see the description in
:ref:`univariate`).
:r_dir:
For "cylindrical" distributions, this element specifies the direction
of the cylinder r-axis at phi=0. Defaults to (1.0, 0.0, 0.0).
:theta:
For a "spherical" distribution, this element specifies the distribution
of theta-coordinates. The necessary sub-elements/attributes are those of a
@ -613,10 +923,39 @@ attributes/sub-elements:
sub-elements/attributes are those of a univariate probability
distribution (see the description in :ref:`univariate`).
:z_dir:
For "cylindrical" distributions, this element specifies the direction
of the cylinder z-axis. Defaults to (0.0, 0.0, 1.0).
:origin:
For "cylindrical and "spherical" distributions, this element specifies
the coordinates for the origin of the coordinate system.
:mesh_id:
For "mesh" spatial distributions, this element specifies which mesh ID to
use for the geometric description of the mesh.
:coords:
For "cloud" distributions, this element specifies a list of coordinates
for each of the points in the cloud.
:strengths:
For "mesh" and "cloud" spatial distributions, this element specifies the
relative source strength of each mesh element or each point in the cloud.
:volume_normalized:
For "mesh" spatial distributions, this optional boolean element specifies
whether the vector of relative strengths should be multiplied by the mesh
element volume. This is most common if the strengths represent a source
per unit volume.
*Default*: false
:bias:
For "mesh" and "cloud" spatial distributions, this optional element
specifies floating point values corresponding to alternative probabilities
for each value/component to use for biased sampling.
:angle:
An element specifying the angular distribution of source sites. This element
has the following attributes:
@ -649,6 +988,10 @@ attributes/sub-elements:
are those of a univariate probability distribution (see the description in
:ref:`univariate`).
:bias:
For "isotropic" angular distributions, this optional element specifies a
"mu-phi" angular distribution used for biased sampling.
:energy:
An element specifying the energy distribution of source sites. The necessary
sub-elements/attributes are those of a univariate probability distribution
@ -664,6 +1007,125 @@ attributes/sub-elements:
*Default*: false
:mesh:
For mesh sources, this indicates the ID of the corresponding mesh.
:source:
For mesh sources, this sub-element specifies the source for an individual
mesh element and follows the format for :ref:`source_element`. The number of
``<source>`` sub-elements should correspond to the number of mesh elements.
For a source with ``type="tokamak"``, the spatial distribution is described by
a Miller-style flux-surface parameterization and the following sub-elements
are used instead of the ``space`` element:
:major_radius:
The major radius :math:`R_0` of the plasma in [cm].
:minor_radius:
The minor radius :math:`a` of the plasma in [cm]. Must be smaller than
``major_radius``.
:elongation:
The plasma elongation :math:`\kappa` (must be > 0).
:triangularity:
The plasma triangularity :math:`\delta` (must be in [-1, 1]). Negative
values describe negative-triangularity plasmas.
:shafranov_shift:
The Shafranov shift :math:`\Delta` in [cm] (must be >= 0 and less than
``minor_radius``/2).
:r_over_a:
A list of normalized minor-radius grid points :math:`r/a`. Must be strictly
increasing, start at 0, and end at 1.
:emission_density:
A list of neutron emission densities :math:`S(r)` evaluated at each
``r_over_a`` grid point (arbitrary units, must be non-negative). Only the
shape matters, since the profile is normalized internally. Values are
interpolated linearly between grid points and the profile is refined on an
internal grid for radial sampling. Must have the same length as
``r_over_a`` and contain at least one positive value.
:phi_start:
The starting toroidal angle in [rad].
*Default*: 0.0
:phi_extent:
The toroidal angle extent in [rad]. The source is sampled uniformly in
:math:`[\phi_\text{start},\ \phi_\text{start} + \phi_\text{extent}]`.
*Default*: :math:`2\pi`
:n_alpha:
The number of poloidal-angle grid points used to build the sampling CDFs
(must be > 2). Larger values reduce discretization bias; values below 51
produce a warning.
*Default*: 101
:vertical_shift:
A vertical shift of the plasma center in [cm].
*Default*: 0.0
:energy:
For a tokamak source, one or more ``energy`` sub-elements specify the
neutron energy distribution(s). Either a single distribution is given (used
at all radii) or exactly one distribution per ``r_over_a`` grid point is
given, in which case the energy is sampled from one of the two
distributions bracketing the sampled radius, selected stochastically with
probability proportional to the proximity of the radius to each grid point
(stochastic interpolation). Each follows the format of a univariate
probability distribution (see :ref:`univariate`).
:time:
An optional ``time`` sub-element specifying the time distribution of source
particles, following the format of a univariate probability distribution
(see :ref:`univariate`).
*Default*: particles are born at :math:`t=0`
.. note:: Biased sampling can be applied to the spatial and energy distributions
of a source by using the ``<bias>`` sub-element (see
:ref:`univariate` for details on how to specify bias distributions).
:constraints:
This sub-element indicates the presence of constraints on sampled source
sites (see :ref:`usersguide_source_constraints` for details). It may have
the following sub-elements:
:domain_ids:
The unique IDs of domains for which source sites must be within.
*Default*: None
:domain_type:
The type of each domain for source rejection ("cell", "material", or
"universe").
*Default*: None
:fissionable:
A boolean indicating whether source sites must be sampled within a
material that is fissionable in order to be accepted.
:time_bounds:
A pair of times in [s] indicating the lower and upper bound for a time
interval that source particles must be within.
:energy_bounds:
A pair of energies in [eV] indicating the lower and upper bound for an
energy interval that source particles must be within.
:rejection_strategy:
Either "resample", indicating that source sites should be resampled when
one is rejected, or "kill", indicating that a rejected source site is
assigned zero weight.
.. _univariate:
Univariate Probability Distributions
@ -677,17 +1139,19 @@ variable and whose sub-elements/attributes are as follows:
:type:
The type of the distribution. Valid options are "uniform", "discrete",
"tabular", "maxwell", "watt", and "mixture". The "uniform" option produces
variates sampled from a uniform distribution over a finite interval. The
"discrete" option produces random variates that can assume a finite number
of values (i.e., a distribution characterized by a probability mass function).
The "tabular" option produces random variates sampled from a tabulated
distribution where the density function is either a histogram or
"tabular", "maxwell", "watt", "mixture", and "decay_spectrum". The "uniform"
option produces variates sampled from a uniform distribution over a finite
interval. The "discrete" option produces random variates that can assume a
finite number of values (i.e., a distribution characterized by a probability
mass function). The "tabular" option produces random variates sampled from a
tabulated distribution where the density function is either a histogram or
linearly-interpolated between tabulated points. The "watt" option produces
random variates is sampled from a Watt fission spectrum (only used for
energies). The "maxwell" option produce variates sampled from a Maxwell
fission spectrum (only used for energies). The "mixture" option produces samples
from univariate sub-distributions with given probabilities.
fission spectrum (only used for energies). The "mixture" option produces
samples from univariate sub-distributions with given probabilities. The
"decay_spectrum" option produces photon energies sampled from decay photon
spectra in a depletion chain (only used for energies).
*Default*: None
@ -705,6 +1169,10 @@ variable and whose sub-elements/attributes are as follows:
:math:`(x,p)` pairs defining the discrete/tabular distribution. All :math:`x`
points are given first followed by corresponding :math:`p` points.
For a "decay_spectrum" distribution, ``parameters`` gives the atom densities
in [atom/b-cm] for the nuclides listed in the ``nuclides`` element, in the
same order.
For a "watt" distribution, ``parameters`` should be given as two real numbers
:math:`a` and :math:`b` that parameterize the distribution :math:`p(x) dx = c
e^{-x/a} \sinh \sqrt{b \, x} dx`.
@ -723,30 +1191,51 @@ variable and whose sub-elements/attributes are as follows:
*Default*: histogram
:pair:
For a "mixture" distribution, this element provides a distribution and its corresponding probability.
For a "mixture" distribution, this element provides a distribution and its
corresponding probability.
:probability:
An attribute or ``pair`` that provides the probability of a univariate distribution within a "mixture" distribution.
An attribute or ``pair`` that provides the probability of a univariate
distribution within a "mixture" distribution.
:dist:
This sub-element of a ``pair`` element provides information on the corresponding univariate distribution.
This sub-element of a ``pair`` element provides information on the
corresponding univariate distribution.
-------------------------
``<state_point>`` Element
-------------------------
:volume:
For a "decay_spectrum" distribution, this attribute specifies the source
region volume in cm\ :sup:`3`. It is used together with atom densities to
determine the absolute photon emission rate. When a source uses a
"decay_spectrum" energy distribution, the source strength is set from this
emission rate.
The ``<state_point>`` element indicates at what batches a state point file
should be written. A state point file can be used to restart a run or to get
tally results at any batch. The default behavior when using this tag is to
write out the source bank in the state_point file. This behavior can be
customized by using the ``<source_point>`` element. This element has the
following attributes/sub-elements:
:nuclides:
For a "decay_spectrum" distribution, this element specifies a
whitespace-separated list of nuclide names contributing to the decay photon
source. The atom densities for these nuclides are given by the ``parameters``
element in the same order. Nuclides are resolved against the depletion chain,
and nuclides without decay photon spectra do not contribute to the
distribution.
:batches:
A list of integers separated by spaces indicating at what batches a state
point file should be written.
:bias:
This optional element specifies a biased distribution for importance sampling.
For continuous distributions, the ``bias`` element should contain another
univariate distribution with the same support (interval) as the parent
distribution. For discrete distributions, the ``bias`` element should contain
floating point values corresponding to alternative probabilities for each
value/component to be used for biased sampling.
*Default*: Last batch only
*Default*: None
---------------------------------------
``<source_rejection_fraction>`` Element
---------------------------------------
The ``<source_rejection_fraction>`` element specifies the minimum fraction of
external source sites that must be accepted when applying rejection sampling
based on constraints.
*Default*: 0.05
--------------------------
``<source_point>`` Element
@ -797,6 +1286,32 @@ attributes/sub-elements:
*Default*: false
-------------------------
``<state_point>`` Element
-------------------------
The ``<state_point>`` element indicates at what batches a state point file
should be written. A state point file can be used to restart a run or to get
tally results at any batch. The default behavior when using this tag is to
write out the source bank in the state_point file. This behavior can be
customized by using the ``<source_point>`` element. This element has the
following attributes/sub-elements:
:batches:
A list of integers separated by spaces indicating at what batches a state
point file should be written.
*Default*: Last batch only
--------------------
``<stride>`` Element
--------------------
The ``stride`` element is used to specify how many random numbers are allocated
for each source particle history.
*Default*: 152,917
------------------------------
``<surf_source_read>`` Element
------------------------------
@ -816,7 +1331,12 @@ attributes/sub-elements:
The ``<surf_source_write>`` element triggers OpenMC to bank particles crossing
certain surfaces and write out the source bank in a separate file called
``surface_source.h5``. This element has the following attributes/sub-elements:
``surface_source.h5``. One or multiple surface IDs and one cell ID can be used
to select the surfaces of interest. If no surface IDs are declared, every surface
of the model is eligible to bank particles. In that case, a cell ID (using
either the ``cell``, ``cellfrom`` or ``cellto`` attributes) can be used to select
every surface of a specific cell. This element has the following
attributes/sub-elements:
:surface_ids:
A list of integers separated by spaces indicating the unique IDs of surfaces
@ -832,6 +1352,15 @@ certain surfaces and write out the source bank in a separate file called
*Default*: None
:max_source_files:
An integer value indicating the number of surface source files to be written
containing the maximum number of particles each. The surface source bank
will be cleared in simulation memory each time a surface source file is
written. By default a ``surface_source.h5`` file will be created when the
maximum number of saved particles is reached.
*Default*: 1
:mcpl:
An optional boolean which indicates if the banked particles should be
written to a file in the MCPL_-format instead of the native HDF5-based
@ -842,6 +1371,51 @@ certain surfaces and write out the source bank in a separate file called
.. _MCPL: https://mctools.github.io/mcpl/mcpl.pdf
:cell:
An integer representing the cell ID used to determine if particles crossing
identified surfaces are to be banked. Particles coming from or going to this
declared cell will be banked if they cross the identified surfaces.
*Default*: None
:cellfrom:
An integer representing the cell ID used to determine if particles crossing
identified surfaces are to be banked. Particles coming from this declared
cell will be banked if they cross the identified surfaces.
*Default*: None
:cellto:
An integer representing the cell ID used to determine if particles crossing
identified surfaces are to be banked. Particles going to this declared cell
will be banked if they cross the identified surfaces.
*Default*: None
.. note:: The ``cell``, ``cellfrom`` and ``cellto`` attributes cannot be
used simultaneously.
.. note:: Surfaces with boundary conditions that are not "transmission" or "vacuum"
are not eligible to store any particles when using ``cell``, ``cellfrom``
or ``cellto`` attributes. It is recommended to use surface IDs instead.
------------------------------------
``<surface_grazing_cutoff>`` Element
------------------------------------
The ``<surface_grazing_cutoff>`` element specifies the surface flux cosine cutoff.
*Default*: 0.001
-----------------------------------
``<surface_grazing_ratio>`` Element
-----------------------------------
The ``<surface_grazing_ratio>`` element specifies the surface flux cosine
substitution ratio.
*Default*: 0.5
------------------------------
``<survival_biasing>`` Element
------------------------------
@ -1025,6 +1599,15 @@ has the following attributes/sub-elements:
for fixed source and small criticality calculations, but is very
optimistic for highly coupled full-core reactor problems.
-------------------------------------
``<uniform_source_sampling>`` Element
-------------------------------------
The ``<uniform_source_sampling>`` element indicates whether to sample among
multiple sources uniformly, applying their strengths as weights to sampled
particles.
*Default*: False
------------------------
``<ufs_mesh>`` Element
@ -1037,6 +1620,16 @@ Agency Monte Carlo Performance Benchmark Problem," Proceedings of *Physor 2012*,
Knoxville, TN (2012). The mesh should cover all possible fissionable materials
in the problem and is specified using a :ref:`mesh_element`.
-------------------------------
``<use_decay_photons>`` Element
-------------------------------
The ``<use_decay_photons>`` element indicates whether to produce decay photons
from neutron reactions instead of prompt photons. This is used in conjunction
with the direct 1-step method for shutdown dose rate calculations.
*Default*: False
.. _verbosity:
-----------------------
@ -1138,7 +1731,8 @@ sub-elements/attributes:
*Default*: None
:particle_type:
The particle that the weight windows will apply to (e.g., 'neutron')
The particle that the weight windows will apply to, specified as a PDG
code or string (e.g., ``neutron``).
*Default*: 'neutron'
@ -1198,7 +1792,8 @@ mesh-based weight windows.
*Default*: None
:particle_type:
The particle that the weight windows will apply to (e.g., 'neutron')
The particle that the weight windows will apply to, specified as a PDG
code or string (e.g., ``neutron``).
*Default*: neutron
@ -1218,7 +1813,7 @@ mesh-based weight windows.
*Default*: true
:method:
Method used to update weight window values (currently only 'magic' is supported)
Method used to update weight window values (one of 'magic' or 'fw_cadis')
*Default*: magic
@ -1242,6 +1837,14 @@ mesh-based weight windows.
*Default*: 5.0
For FW-CADIS:
:targets:
A sequence of IDs corresponding to the tallies which cover phase
space regions of interest for local variance reduction.
*Default*: None
---------------------------------------
``<weight_window_checkpoints>`` Element
---------------------------------------
@ -1267,3 +1870,21 @@ following sub-elements/attributes:
The ``weight_windows_file`` element has no attributes and contains the path to
a weight windows HDF5 file to load during simulation initialization.
-------------------------------
``<weight_windows_on>`` Element
-------------------------------
The ``weight_windows_on`` element indicates whether weight windows are
enabled.
*Default*: False
----------------------------------
``<write_initial_source>`` Element
----------------------------------
The ``write_initial_source`` element indicates whether to write the initial
source distribution to file.
*Default*: False

View file

@ -15,6 +15,8 @@ following the same format.
**/**
:Attributes: - **filetype** (*char[]*) -- String indicating the type of file.
- **version** (*int[2]*) -- Major and minor version of the source
file format.
:Datasets:
@ -22,5 +24,5 @@ following the same format.
particle. The compound type has fields ``r``, ``u``, ``E``,
``time``, ``wgt``, ``delayed_group``, ``surf_id`` and ``particle``,
which represent the position, direction, energy, time, weight,
delayed group, surface ID, and particle type (0=neutron, 1=photon,
2=electron, 3=positron), respectively.
delayed group, surface ID, and particle type (PDG number),
respectively.

View file

@ -4,7 +4,7 @@
State Point File Format
=======================
The current version of the statepoint file format is 18.1.
The current version of the statepoint file format is 18.2.
**/**
@ -23,6 +23,7 @@ The current version of the statepoint file format is 18.1.
bank is present (1) or not (0).
:Datasets: - **seed** (*int8_t*) -- Pseudo-random number generator seed.
- **stride** (*uint64_t*) -- Pseudo-random number generator stride.
- **energy_mode** (*char[]*) -- Energy mode of the run, either
'continuous-energy' or 'multi-group'.
- **run_mode** (*char[]*) -- Run mode used, either 'eigenvalue' or
@ -55,8 +56,8 @@ The current version of the statepoint file format is 18.1.
``time``, ``wgt``, ``delayed_group``, ``surf_id``, and
``particle``, which represent the position, direction, energy,
time, weight, delayed group, surface ID, and particle type
(0=neutron, 1=photon, 2=electron, 3=positron), respectively. Only
present when `run_mode` is 'eigenvalue'.
(PDG number), respectively. Only present when `run_mode` is
'eigenvalue'.
**/tallies/**
@ -72,7 +73,10 @@ The current version of the statepoint file format is 18.1.
**/tallies/meshes/mesh <uid>/**
:Datasets: - **type** (*char[]*) -- Type of mesh.
:Attributes: - **id** (*int*) -- ID of the mesh
:Datasets: - **name** (*char[]*) -- Name of the mesh.
- **type** (*char[]*) -- Type of mesh.
- **dimension** (*int*) -- Number of mesh cells in each dimension.
- **Regular Mesh Only:**
- **lower_left** (*double[]*) -- Coordinates of lower-left corner of
@ -96,6 +100,8 @@ The current version of the statepoint file format is 18.1.
- **library** (*char[]*) -- Mesh library used to represent the
mesh ("moab" or "libmesh").
- **length_multiplier** (*double*) Scaling factor applied to the mesh.
- **options** (*char[]*) -- Special options that control spatial
search data structures used.
- **volumes** (*double[]*) -- Volume of each mesh cell.
- **vertices** (*double[]*) -- x, y, z values of the mesh vertices.
- **connectivity** (*int[]*) -- Connectivity array for the mesh
@ -143,6 +149,8 @@ The current version of the statepoint file format is 18.1.
tallies will have a value of 0 unless otherwise instructed.
- **multiply_density** (*int*) -- Flag indicating whether reaction
rates should be multiplied by atom density (1) or not (0).
- **higher_moments** (*int*) -- Flag indicating whether
higher-order tally moments are enabled (1) or not (0).
:Datasets: - **n_realizations** (*int*) -- Number of realizations.
- **n_filters** (*int*) -- Number of filters used.

View file

@ -4,7 +4,7 @@
Summary File Format
===================
The current version of the summary file format is 6.0.
The current version of the summary file format is 6.1.
**/**
@ -38,6 +38,7 @@ The current version of the summary file format is 6.0.
is an array if the cell uses distributed materials, otherwise it is
a scalar.
- **temperature** (*double[]*) -- Temperature of the cell in Kelvin.
- **density** (*double[]*) -- Density of the cell in [g/cm3].
- **translation** (*double[3]*) -- Translation applied to the fill
universe. This dataset is present only if fill_type is set to
'universe'.

View file

@ -100,6 +100,18 @@ The ``<tally>`` element accepts the following sub-elements:
*Default*: None
:ignore_zeros:
Whether to allow zero tally bins to be ignored when assessing the
convergece of the precision trigger. If True, only nonzero tally scores
will be compared to the trigger's threshold.
.. note:: The ``ignore_zeros`` option can cause the tally trigger to fire
prematurely if there are no hits in any bins at the first
evalulation. It is the user's responsibility to specify enough
particles per batch to get a nonzero score in at least one bin.
*Default*: False
:scores:
The score(s) in this tally to which the trigger should be applied.
@ -130,9 +142,9 @@ attributes/sub-elements:
:type:
The type of the filter. Accepted options are "cell", "cellfrom",
"cellborn", "surface", "material", "universe", "energy", "energyout", "mu",
"polar", "azimuthal", "mesh", "distribcell", "delayedgroup",
"energyfunction", and "particle".
"cellborn", "surface", "material", "universe", "energy", "energyout",
"mu", "polar", "azimuthal", "mesh", "distribcell", "delayedgroup",
"energyfunction", "particle", and "particleproduction".
:bins:
A description of the bins for each type of filter can be found in
@ -306,8 +318,34 @@ should be set to:
they use ``energy`` and ``y``.
:particle:
A list of integers indicating the type of particles to tally ('neutron' = 1,
'photon' = 2, 'electron' = 3, 'positron' = 4).
A list of particle identifiers to tally, specified as strings (e.g.,
``neutron``, ``photon``, ``He4``) or as integer PDG numbers.
:particleproduction:
This filter tallies secondary particles produced in reactions, binned by
particle type and, optionally, by energy. Unlike other energy filters, the
weight applied is the weight of the secondary particle. To obtain secondary
particle production rates, use this filter with the ``events`` score.
The filter uses the following sub-elements instead of ``bins``:
:particles:
A space-separated list of secondary particle types to tally (e.g.,
``photon``, ``neutron``, ``electron``).
:energies:
An optional monotonically increasing list of energy boundaries in [eV]
for binning the secondary particle energies. If omitted, total production
is tallied without energy binning.
For example, to tally photon and neutron production in three energy groups:
.. code-block:: xml
<filter id="1" type="particleproduction">
<particles>photon neutron</particles>
<energies>0.0 1.0e5 1.0e6 20.0e6</energies>
</filter>
------------------
``<mesh>`` Element
@ -317,6 +355,11 @@ If a mesh is desired as a filter for a tally, it must be specified in a separate
element with the tag name ``<mesh>``. This element has the following
attributes/sub-elements:
:name:
An optional string name to identify the mesh in output files.
*Default*: ""
:type:
The type of mesh. This can be either "regular", "rectilinear",
"cylindrical", "spherical", or "unstructured".
@ -364,6 +407,10 @@ attributes/sub-elements:
The mesh library used to represent an unstructured mesh. This can be either
"moab" or "libmesh". (For unstructured mesh only.)
:options:
Special options that control spatial search data structures used. (For
unstructured mesh using MOAB only)
:filename:
The name of the mesh file to be loaded at runtime. (For unstructured mesh
only.)

View file

@ -4,7 +4,7 @@
Track File Format
=================
The current revision of the particle track file format is 3.0.
The current revision of the particle track file format is 3.1.
**/**
@ -32,6 +32,5 @@ The current revision of the particle track file format is 3.0.
the array for each primary/secondary particle. The
last offset should match the total size of the
array.
- **particles** (*int[]*) -- Particle type for each
primary/secondary particle (0=neutron, 1=photon,
2=electron, 3=positron).
- **particles** (*int32_t[]*) -- Particle type for
each primary/secondary particle (PDG number).

View file

@ -4,7 +4,7 @@
License Agreement
=================
Copyright © 2011-2023 Massachusetts Institute of Technology, UChicago Argonne
Copyright © 2011-2026 Massachusetts Institute of Technology, UChicago Argonne
LLC, and OpenMC contributors
Permission is hereby granted, free of charge, to any person obtaining a copy of

View file

@ -0,0 +1,362 @@
.. _methods_charged_particle_physics:
========================
Charged Particle Physics
========================
OpenMC neglects the spatial transport of charged particles (electrons and
positrons), assuming they deposit all their energy locally and produce
bremsstrahlung photons at their birth location. This approximation, called
thick-target bremsstrahlung (TTB) approximation is justified by the fact that
charged particles have much shorter stopping ranges compared to neutrons and
photons, especially in high-density materials.
-----------------------------
Charged Particle Interactions
-----------------------------
Bremsstrahlung
--------------
When a charged particle is decelerated in the field of an atom, some of its
kinetic energy is converted into electromagnetic radiation known as
bremsstrahlung, or 'braking radiation'. In each event, an electron or positron
with kinetic energy :math:`T` generates a photon with an energy :math:`E`
between :math:`0` and :math:`T`. Bremsstrahlung is described by a cross section
that is differential in photon energy, in the direction of the emitted photon,
and in the final direction of the charged particle. However, in Monte Carlo
simulations it is typical to integrate over the angular variables to obtain a
single differential cross section with respect to photon energy, which is often
expressed in the form
.. math::
:label: bremsstrahlung-dcs
\frac{d\sigma_{\text{br}}}{dE} = \frac{Z^2}{\beta^2} \frac{1}{E}
\chi(Z, T, \kappa),
where :math:`\kappa = E/T` is the reduced photon energy and :math:`\chi(Z, T,
\kappa)` is the scaled bremsstrahlung cross section, which is experimentally
measured.
Because electrons are attracted to atomic nuclei whereas positrons are
repulsed, the cross section for positrons is smaller, though it approaches that
of electrons in the high energy limit. To obtain the positron cross section, we
multiply :eq:`bremsstrahlung-dcs` by the :math:`\kappa`-independent factor used
in Salvat_,
.. math::
:label: positron-factor
\begin{aligned}
F_{\text{p}}(Z,T) =
& 1 - \text{exp}(-1.2359\times 10^{-1}t + 6.1274\times 10^{-2}t^2 - 3.1516\times 10^{-2}t^3 \\
& + 7.7446\times 10^{-3}t^4 - 1.0595\times 10^{-3}t^5 + 7.0568\times 10^{-5}t^6 \\
& - 1.8080\times 10^{-6}t^7),
\end{aligned}
where
.. math::
:label: positron-factor-t
t = \ln\left(1 + \frac{10^6}{Z^2}\frac{T}{\text{m}_\text{e}c^2} \right).
:math:`F_{\text{p}}(Z,T)` is the ratio of the radiative stopping powers for
positrons and electrons. Stopping power describes the average energy loss per
unit path length of a charged particle as it passes through matter:
.. math::
:label: stopping-power
-\frac{dT}{ds} = n \int E \frac{d\sigma}{dE} dE \equiv S(T),
where :math:`n` is the number density of the material and :math:`d\sigma/dE` is
the cross section differential in energy loss. The total stopping power
:math:`S(T)` can be separated into two components: the radiative stopping
power :math:`S_{\text{rad}}(T)`, which refers to energy loss due to
bremsstrahlung, and the collision stopping power :math:`S_{\text{col}}(T)`,
which refers to the energy loss due to inelastic collisions with bound
electrons in the material that result in ionization and excitation. The
radiative stopping power for electrons is given by
.. math::
:label: radiative-stopping-power
S_{\text{rad}}(T) = n \frac{Z^2}{\beta^2} T \int_0^1 \chi(Z,T,\kappa)
d\kappa.
To obtain the radiative stopping power for positrons,
:eq:`radiative-stopping-power` is multiplied by :eq:`positron-factor`.
While the models for photon interactions with matter described above can safely
assume interactions occur with free atoms, sampling the target atom based on
the macroscopic cross sections, molecular effects cannot necessarily be
disregarded for charged particle treatment. For compounds and mixtures, the
bremsstrahlung cross section is calculated using Bragg's additivity rule as
.. math::
:label: material-bremsstrahlung-dcs
\frac{d\sigma_{\text{br}}}{dE} = \frac{1}{\beta^2 E} \sum_i \gamma_i Z^2_i
\chi(Z_i, T, \kappa),
where the sum is over the constituent elements and :math:`\gamma_i` is the
atomic fraction of the :math:`i`-th element. Similarly, the radiative stopping
power is calculated using Bragg's additivity rule as
.. math::
:label: material-radiative-stopping-power
S_{\text{rad}}(T) = \sum_i w_i S_{\text{rad},i}(T),
where :math:`w_i` is the mass fraction of the :math:`i`-th element and
:math:`S_{\text{rad},i}(T)` is found for element :math:`i` using
:eq:`radiative-stopping-power`. The collision stopping power, however, is a
function of certain quantities such as the mean excitation energy :math:`I` and
the density effect correction :math:`\delta_F` that depend on molecular
properties. These quantities cannot simply be summed over constituent elements
in a compound, but should instead be calculated for the material. The Bethe
formula can be used to find the collision stopping power of the material:
.. math::
:label: material-collision-stopping-power
S_{\text{col}}(T) = \frac{2 \pi r_e^2 m_e c^2}{\beta^2} N_A \frac{Z}{A_M}
[\ln(T^2/I^2) + \ln(1 + \tau/2) + F(\tau) - \delta_F(T)],
where :math:`N_A` is Avogadro's number, :math:`A_M` is the molar mass,
:math:`\tau = T/m_e`, and :math:`F(\tau)` depends on the particle type. For
electrons,
.. math::
:label: F-electron
F_{-}(\tau) = (1 - \beta^2)[1 + \tau^2/8 - (2\tau + 1) \ln2],
while for positrons
.. math::
:label: F-positron
F_{+}(\tau) = 2\ln2 - (\beta^2/12)[23 + 14/(\tau + 2) + 10/(\tau + 2)^2 +
4/(\tau + 2)^3].
The density effect correction :math:`\delta_F` takes into account the reduction
of the collision stopping power due to the polarization of the material the
charged particle is passing through by the electric field of the particle.
It can be evaluated using the method described by Sternheimer_, where the
equation for :math:`\delta_F` is
.. math::
:label: density-effect-correction
\delta_F(\beta) = \sum_{i=1}^n f_i \ln[(l_i^2 + l^2)/l_i^2] -
l^2(1-\beta^2).
Here, :math:`f_i` is the oscillator strength of the :math:`i`-th transition,
given by :math:`f_i = n_i/Z`, where :math:`n_i` is the number of electrons in
the :math:`i`-th subshell. The frequency :math:`l` is the solution of the
equation
.. math::
:label: density-effect-l
\frac{1}{\beta^2} - 1 = \sum_{i=1}^{n} \frac{f_i}{\bar{\nu}_i^2 + l^2},
where :math:`\bar{v}_i` is defined as
.. math::
:label: density-effect-nubar
\bar{\nu}_i = h\nu_i \rho / h\nu_p.
The plasma energy :math:`h\nu_p` of the medium is given by
.. math::
:label: plasma-frequency
h\nu_p = \sqrt{\frac{(hc)^2 r_e \rho_m N_A Z}{\pi A}},
where :math:`A` is the atomic weight and :math:`\rho_m` is the density of the
material. In :eq:`density-effect-nubar`, :math:`h\nu_i` is the oscillator
energy, and :math:`\rho` is an adjustment factor introduced to give agreement
between the experimental values of the oscillator energies and the mean
excitation energy. The :math:`l_i` in :eq:`density-effect-correction` are
defined as
.. math::
:label: density-effect-li
\begin{aligned}
l_i &= (\bar{\nu}_i^2 + 2/3f_i)^{1/2} ~~~~&\text{for}~~ \bar{\nu}_i > 0 \\
l_n &= f_n^{1/2} ~~~~&\text{for}~~ \bar{\nu}_n = 0,
\end{aligned}
where the second case applies to conduction electrons. For a conductor,
:math:`f_n` is given by :math:`n_c/Z`, where :math:`n_c` is the effective
number of conduction electrons, and :math:`v_n = 0`. The adjustment factor
:math:`\rho` is determined using the equation for the mean excitation energy:
.. math::
:label: mean-excitation-energy
\ln I = \sum_{i=1}^{n-1} f_i \ln[(h\nu_i\rho)^2 + 2/3f_i(h\nu_p)^2]^{1/2} +
f_n \ln (h\nu_pf_n^{1/2}).
.. _ttb:
Thick-Target Bremsstrahlung Approximation
+++++++++++++++++++++++++++++++++++++++++
Since charged particles lose their energy on a much shorter distance scale than
neutral particles, not much error should be introduced by neglecting to
transport electrons. However, the bremsstrahlung emitted from high energy
electrons and positrons can travel far from the interaction site. Thus, even
without a full electron transport mode it is necessary to model bremsstrahlung.
We use a thick-target bremsstrahlung (TTB) approximation based on the models in
Salvat_ and Kaltiaisenaho_ for generating bremsstrahlung photons, which assumes
the charged particle loses all its energy in a single homogeneous material
region.
To model bremsstrahlung using the TTB approximation, we need to know the number
of photons emitted by the charged particle and the energy distribution of the
photons. These quantities can be calculated using the continuous slowing down
approximation (CSDA). The CSDA assumes charged particles lose energy
continuously along their trajectory with a rate of energy loss equal to the
total stopping power, ignoring fluctuations in the energy loss. The
approximation is useful for expressing average quantities that describe how
charged particles slow down in matter. For example, the CSDA range approximates
the average path length a charged particle travels as it slows to rest:
.. math::
:label: csda-range
R(T) = \int^T_0 \frac{dT'}{S(T')}.
Actual path lengths will fluctuate around :math:`R(T)`. The average number of
photons emitted per unit path length is given by the inverse bremsstrahlung
mean free path:
.. math::
:label: inverse-bremsstrahlung-mfp
\lambda_{\text{br}}^{-1}(T,E_{\text{cut}})
= n\int_{E_{\text{cut}}}^T\frac{d\sigma_{\text{br}}}{dE}dE
= n\frac{Z^2}{\beta^2}\int_{\kappa_{\text{cut}}}^1\frac{1}{\kappa}
\chi(Z,T,\kappa)d\kappa.
The lower limit of the integral in :eq:`inverse-bremsstrahlung-mfp` is non-zero
because the bremsstrahlung differential cross section diverges for small photon
energies but is finite for photon energies above some cutoff energy
:math:`E_{\text{cut}}`. The mean free path
:math:`\lambda_{\text{br}}^{-1}(T,E_{\text{cut}})` is used to calculate the
photon number yield, defined as the average number of photons emitted with
energy greater than :math:`E_{\text{cut}}` as the charged particle slows down
from energy :math:`T` to :math:`E_{\text{cut}}`. The photon number yield is
given by
.. math::
:label: photon-number-yield
Y(T,E_{\text{cut}}) = \int^{R(T)}_{R(E_{\text{cut}})}
\lambda_{\text{br}}^{-1}(T',E_{\text{cut}})ds = \int_{E_{\text{cut}}}^T
\frac{\lambda_{\text{br}}^{-1}(T',E_{\text{cut}})}{S(T')}dT'.
:math:`Y(T,E_{\text{cut}})` can be used to construct the energy spectrum of
bremsstrahlung photons: the number of photons created with energy between
:math:`E_1` and :math:`E_2` by a charged particle with initial kinetic energy
:math:`T` as it comes to rest is given by :math:`Y(T,E_1) - Y(T,E_2)`.
To simulate the emission of bremsstrahlung photons, the total stopping power
and bremsstrahlung differential cross section for positrons and electrons must
be calculated for a given material using :eq:`material-bremsstrahlung-dcs` and
:eq:`material-radiative-stopping-power`. These quantities are used to build the
tabulated bremsstrahlung energy PDF and CDF for that material for each incident
energy :math:`T_k` on the energy grid. The following algorithm is then applied
to sample the photon energies:
1. For an incident charged particle with energy :math:`T`, sample the number of
emitted photons as
.. math::
N = \lfloor Y(T,E_{\text{cut}}) + \xi_1 \rfloor.
2. Rather than interpolate the PDF between indices :math:`k` and :math:`k+1`
for which :math:`T_k < T < T_{k+1}`, which is computationally expensive, use
the composition method and sample from the PDF at either :math:`k` or
:math:`k+1`. Using linear interpolation on a logarithmic scale, the PDF can
be expressed as
.. math::
p_{\text{br}}(T,E) = \pi_k p_{\text{br}}(T_k,E) + \pi_{k+1}
p_{\text{br}}(T_{k+1},E),
where the interpolation weights are
.. math::
\pi_k = \frac{\ln T_{k+1} - \ln T}{\ln T_{k+1} - \ln T_k},~~~
\pi_{k+1} = \frac{\ln T - \ln T_k}{\ln T_{k+1} - \ln T_k}.
Sample either the index :math:`i = k` or :math:`i = k+1` according to the
point probabilities :math:`\pi_{k}` and :math:`\pi_{k+1}`.
3. Determine the maximum value of the CDF :math:`P_{\text{br,max}}`.
3. Sample the photon energies using the inverse transform method with the
tabulated CDF :math:`P_{\text{br}}(T_i, E)` i.e.,
.. math::
E = E_j \left[ (1 + a_j) \frac{\xi_2 P_{\text{br,max}} -
P_{\text{br}}(T_i, E_j)} {E_j p_{\text{br}}(T_i, E_j)} + 1
\right]^{\frac{1}{1 + a_j}}
where the interpolation factor :math:`a_j` is given by
.. math::
a_j = \frac{\ln p_{\text{br}}(T_i,E_{j+1}) - \ln p_{\text{br}}(T_i,E_j)}
{\ln E_{j+1} - \ln E_j}
and :math:`P_{\text{br}}(T_i, E_j) \le \xi_2 P_{\text{br,max}} \le
P_{\text{br}}(T_i, E_{j+1})`.
We ignore the range of the electron or positron, i.e., the bremsstrahlung
photons are produced in the same location that the charged particle was
created. The direction of the photons is assumed to be the same as the
direction of the incident charged particle, which is a reasonable approximation
at higher energies when the bremsstrahlung radiation is emitted at small
angles.
Electron-Positron Annihilation
------------------------------
When a positron collides with an electron, both particles are annihilated and
generally two photons with equal energy are created. If the kinetic energy of
the positron is high enough, the two photons can have different energies, and
the higher-energy photon is emitted preferentially in the direction of flight
of the positron. It is also possible to produce a single photon if the
interaction occurs with a bound electron, and in some cases three (or, rarely,
even more) photons can be emitted. However, the annihilation cross section is
largest for low-energy positrons, and as the positron energy decreases, the
angular distribution of the emitted photons becomes isotropic.
In OpenMC, we assume the most likely case in which a low-energy positron (which
has already lost most of its energy to bremsstrahlung radiation) interacts with
an electron which is free and at rest. Two photons with energy equal to the
electron rest mass energy :math:`m_e c^2 = 0.511` MeV are emitted isotropically
in opposite directions.
.. _Kaltiaisenaho: https://aaltodoc.aalto.fi/bitstream/handle/123456789/21004/master_Kaltiaisenaho_Toni_2016.pdf
.. _Salvat: https://doi.org/10.1787/32da5043-en
.. _Sternheimer: https://doi.org/10.1103/PhysRevB.26.6067

View file

@ -289,17 +289,59 @@ sections. This allows flexibility for the model to use highly anisotropic
scattering information in the water while the fuel can be simulated with linear
or even isotropic scattering.
Particle Speed
--------------
When using a multigroup representation of cross sections, the particle speed has
meaning only in an average sense. The particle speed is important when modeling
dynamic behavior. OpenMC calculates the particle speed using the inverse
velocity multigroup data if it is available. If such data is not available,
OpenMC uses an approximate velocity using the group energy bounds in the
following way:
.. math::
\frac{1}{v_g} = \int_{E_{\text{min}}^g}^{E_{\text{max}}^g} \frac{1}{v(E)} \frac{\alpha}{E} dE
Where :math:`E_{\text{min}}^g` and :math:`E_{\text{max}}^g` are the group energy
boundaries for group :math:`g`. :math:`v(E)` is the neutron velocity calculated
using relativistic kinematics, :math:`\alpha` is a normalization constant for the
:math:`\frac{1}{E}` spectrum.
This equation is valid when inside the group boundaries the neutron spectrum
follows a typical :math:`\frac{1}{E}` slowing down spectrum. This assumption is
widely used when generating fine group neutron cross section data libraries from
continuous energy data.
The solution to this equation is:
.. math::
\frac{1}{v_g} = \frac{1}{c \log\left(\frac{E_{\text{max}}^g}{E_{\text{min}}^g}\right)}
\left[ 2(\operatorname{arctanh}(k_{\text{max}}^{-1}) - \operatorname{arctanh}(k_{\text{min}}^{-1}))
- (k_{\text{max}}-k_{\text{min}}) \right]
where :math:`c` is the speed of light and :math:`k_{\text{max}}`,
:math:`k_{\text{min}}` are defined by a change of variables:
.. math::
k = \sqrt{1+\frac{2 m_n c^2}{E}}
where :math:`E` is the particle kinetic energy and :math:`m_n` is the neutron
rest mass.
.. _logarithmic mapping technique:
https://laws.lanl.gov/vhosts/mcnp.lanl.gov/pdf_files/la-ur-14-24530.pdf
https://mcnp.lanl.gov/pdf_files/TechReport_2014_LANL_LA-UR-14-24530_Brown.pdf
.. _Hwang: https://doi.org/10.13182/NSE87-A16381
.. _Josey: https://doi.org/10.1016/j.jcp.2015.08.013
.. _WMP Library: https://github.com/mit-crpg/WMP_Library
.. _MCNP: https://mcnp.lanl.gov
.. _Serpent: http://montecarlo.vtt.fi
.. _NJOY: https://www.njoy21.io/NJOY21/
.. _Serpent: https://serpent.vtt.fi
.. _NJOY: https://www.njoy21.io/
.. _ENDF/B data: https://www.nndc.bnl.gov/endf-b8.0/
.. _Leppanen: https://doi.org/10.1016/j.anucene.2009.03.019
.. _algorithms: http://ab-initio.mit.edu/wiki/index.php/Faddeeva_Package
.. _algorithms: http://ab-initio.mit.edu/faddeeva/
.. _NCrystal: https://github.com/mctools/ncrystal
.. _NCrystal paper: https://doi.org/10.1016/j.cpc.2019.07.015
.. _using plugins: https://doi.org/10.1016/j.cpc.2021.108082

View file

@ -114,7 +114,7 @@ The predictor method only requires one evaluation and its error converges as
twice as expensive as the predictor method, but achieves an error of
:math:`\mathcal{O}(h^2)`. An exhaustive description of time integration methods
and their merits can be found in the `thesis of Colin Josey
<http://dspace.mit.edu/handle/1721.1/7582>`_.
<https://dspace.mit.edu/handle/1721.1/7582>`_.
OpenMC does not rely on a single time integration method but rather has several
classes that implement different algorithms. For example, the

View file

@ -55,15 +55,17 @@ in :ref:`fission-bank-algorithms`.
Source Convergence Issues
-------------------------
.. _methods-shannon-entropy:
Diagnosing Convergence with Shannon Entropy
-------------------------------------------
As discussed earlier, it is necessary to converge both :math:`k_{eff}` and the
source distribution before any tallies can begin. Moreover, the convergence rate
of the source distribution is in general slower than that of
:math:`k_{eff}`. One should thus examine not only the convergence of
:math:`k_{eff}` but also the convergence of the source distribution in order to
make decisions on when to start active batches.
of the source distribution is in general slower than that of :math:`k_{eff}`.
One should thus examine not only the convergence of :math:`k_{eff}` but also the
convergence of the source distribution in order to make decisions on when to
start active batches.
However, the representation of the source distribution makes it a bit more
difficult to analyze its convergence. Since :math:`k_{eff}` is a scalar
@ -108,6 +110,13 @@ at plots of :math:`k_{eff}` and the Shannon entropy. A number of methods have
been proposed (see e.g. [Romano]_, [Ueki]_), but each of these is not without
problems.
Shannon entropy is calculated differently for the random ray solver, as
described :ref:`in the random ray theory section
<methods-shannon-entropy-random-ray>`. Additionally, as the Shannon entropy only
serves as a diagnostic tool for convergence of the fission source distribution,
there is currently no diagnostic to determine if the scattering source
distribution in random ray is converged.
---------------------------
Uniform Fission Site Method
---------------------------
@ -142,7 +151,7 @@ than unity. By ensuring that the expected number of fission sites in each mesh
cell is constant, the collision density across all cells, and hence the variance
of tallies, is more uniform than it would be otherwise.
.. _Shannon entropy: https://laws.lanl.gov/vhosts/mcnp.lanl.gov/pdf_files/la-ur-06-3737.pdf
.. _Shannon entropy: https://mcnp.lanl.gov/pdf_files/TechReport_2006_LANL_LA-UR-06-3737_Brown.pdf
.. [Lieberoth] J. Lieberoth, "A Monte Carlo Technique to Solve the Static
Eigenvalue Problem of the Boltzmann Transport Equation," *Nukleonik*, **11**,

View file

@ -25,19 +25,38 @@ KERMA (Kinetic Energy Release in Materials) [Mack97]_ coefficients for reaction
:math:`\times` cross-section (e.g., eV-barn) and can be used much like a reaction
cross section for the purpose of tallying energy deposition.
KERMA coefficients can be computed using the energy-balance method with
a nuclear data processing code like NJOY, which performs the following
iteration over all reactions :math:`r` for all isotopes :math:`i`
requested
KERMA coefficients can be computed using the energy-balance method with a
nuclear data processing code like NJOY, which estimates the KERMA coefficients
using the following equation:
.. math::
k_{i, r}(E) = \left(E + Q_{i, r} - \bar{E}_{i, r, n}
k_{i, r}(E) = \left(E + Q_{i, r} - \sum\limits_x \bar{E}_{i, r, x}
\right)\sigma_{i, r}(E),
where the summation is over each secondary particle type :math:`x`. This
equation states that the energy deposited is equal to the energy of the incident
particle plus the reaction :math:`Q` value less the energy of secondary
particles that are transported away from the reaction site. For neutron
interactions, the energy-balance KERMA coefficient is
.. math::
k_{i, r}(E) = \left(E + Q_{i, r} - \sum\limits_x \bar{E}_{i, r, n}
- \bar{E}_{i, r, \gamma}\right)\sigma_{i, r}(E),
removing the energy of neutral particles (neutrons and photons) that are
transported away from the reaction site :math:`\bar{E}`, and the reaction
:math:`Q` value.
where :math:`\bar{E}_{i, r, n}` is the average energy of secondary neutrons and
:math:`\bar{E}_{i, r, \gamma}` is the average energy of secondary photons. For
photon and charged particle interactions the KERMA coefficient is
.. math::
:label: energy-balance-photon
k_{i, r}(E) = \left(E + Q_{i, r} - \sum\limits_x \bar{E}_{i, r, x}
\right)\sigma_{i, r}(E).
where the :math:`Q` value is zero for all interactions except for pair
production and positron annihilation.
-------
Fission
@ -120,7 +139,7 @@ run with :math:`N918` reflecting fission heating computed from NJOY.
This modified heating data is stored as the MT=901 reaction and will be scored
if ``heating-local`` is included in :attr:`openmc.Tally.scores`.
Coupled neutron-photon transport
Coupled Neutron-Photon Transport
--------------------------------
Here, OpenMC instructs ``heatr`` to assume that energy from photons is not
@ -138,6 +157,50 @@ Let :math:`N301` represent the total heating number returned from this
This modified heating data is stored as the MT=301 reaction and will be scored
if ``heating`` is included in :attr:`openmc.Tally.scores`.
Photons and Charged Particles
-----------------------------
In OpenMC, energy deposition from photons or charged particles is scored using
the energy balance method based on Equation :eq:`energy-balance-photon`. Special
consideration is given to electrons and positrons as described below.
+++++++++++++++++
Charged Particles
+++++++++++++++++
OpenMC tracks photons interaction by interaction so the energy deposited in each
collision is easily attributed back to the nuclide and reaction for which the
photon interacted with. Charged particles (electrons and photons) aren't tracked
in the same way. For charged particles, OpenMC assumes that all their energy
(less the energy of bremsstrahlung radiation) is deposited in the material in
which they were born. In this way it is harder to trace how much energy should
be attributed in each nuclide.
According to the CSDA approximation (see :ref:`ttb`) the energy deposited by a
charged particle with kinetic energy :math:`T` in the :math:`i`-th element can
be calculated as:
.. math::
E_{i} = \int_{0}^{R(T)} w_{i}S_{\text{col,i}} dx
where :math:`R(T)` is the CSDA range of the charged particle,
:math:`S_{\text{col},i}` is the collision stopping power of the charged particle
in the :math:`i`-th element and :math:`w_i` is the mass fraction of the
:math:`i`-th element. According to the Bethe formula the collision stopping
power of the :math:`i`-th element is proportional to :math:`Z_i/A_i`, so the
fractional collision stopping power from the :math:`i`-th element is:
.. math::
\frac{w_{i}S_{\text{col},i}(T)}{S_{\text{col}}(T)} =
\frac{\frac{w_{i}Z_{i}}{A_{i}}}{\sum_{i}\frac{w_{i}Z_{i}}{A_{i}}} =
\frac{\gamma_i Z_{i}}{\sum_{i}\gamma_i Z_{i}}.
where :math:`\gamma_i` is the atomic fraction of the :math:`i`-th element.
Therefore, the energy deposited by charged particles should be attributed to
a given element according to its fractional charge density.
----------
References
----------

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@ -1066,5 +1066,5 @@ surface is known as in :ref:`reflection`.
.. _constructive solid geometry: https://en.wikipedia.org/wiki/Constructive_solid_geometry
.. _surfaces: https://en.wikipedia.org/wiki/Surface
.. _MCNP: https://mcnp.lanl.gov
.. _Serpent: http://montecarlo.vtt.fi
.. _Serpent: https://serpent.vtt.fi
.. _Monte Carlo Performance benchmark: https://github.com/mit-crpg/benchmarks/tree/master/mc-performance/openmc

View file

@ -14,9 +14,12 @@ Theory and Methodology
random_numbers
neutron_physics
photon_physics
charged_particles_physics
tallies
eigenvalue
depletion
energy_deposition
parallelization
cmfd
variance_reduction
random_ray

View file

@ -290,7 +290,10 @@ create and store fission sites for the following generation. First, the average
number of prompt and delayed neutrons must be determined to decide whether the
secondary neutrons will be prompt or delayed. This is important because delayed
neutrons have a markedly different spectrum from prompt neutrons, one that has a
lower average energy of emission. The total number of neutrons emitted
lower average energy of emission. Furthermore, in simulations where tracking
time of neutrons is important, we need to consider the emission time delay of
the secondary neutrons, which is dependent on the decay constant of the
delayed neutron precursor. The total number of neutrons emitted
:math:`\nu_t` is given as a function of incident energy in the ENDF format. Two
representations exist for :math:`\nu_t`. The first is a polynomial of order
:math:`N` with coefficients :math:`c_0,c_1,\dots,c_N`. If :math:`\nu_t` has this
@ -306,8 +309,8 @@ interpolation law. The number of prompt neutrons released per fission event
:math:`\nu_p` is also given as a function of incident energy and can be
specified in a polynomial or tabular format. The number of delayed neutrons
released per fission event :math:`\nu_d` can only be specified in a tabular
format. In practice, we only need to determine :math:`nu_t` and
:math:`nu_d`. Once these have been determined, we can calculated the delayed
format. In practice, we only need to determine :math:`\nu_t` and
:math:`\nu_d`. Once these have been determined, we can calculate the delayed
neutron fraction
.. math::
@ -335,8 +338,14 @@ neutrons. Otherwise, we produce :math:`\lfloor \nu \rfloor + 1` neutrons. Then,
for each fission site produced, we sample the outgoing angle and energy
according to the algorithms given in :ref:`sample-angle` and
:ref:`sample-energy` respectively. If the neutron is to be born delayed, then
there is an extra step of sampling a delayed neutron precursor group since they
each have an associated secondary energy distribution.
there is an extra step of sampling a delayed neutron precursor group to get the
associated secondary energy distribution and the decay constant
:math:`\lambda`, which is needed to sample the emission delay time :math:`t_d`:
.. math::
:label: sample-delay-time
t_d = -\frac{\ln \xi}{\lambda}.
The sampled outgoing angle and energy of fission neutrons along with the
position of the collision site are stored in an array called the fission
@ -1743,19 +1752,19 @@ types.
.. _Watt fission spectrum: https://doi.org/10.1103/PhysRev.87.1037
.. _Foderaro: http://hdl.handle.net/1721.1/1716
.. _Foderaro: https://dspace.mit.edu/handle/1721.1/1716
.. _OECD: https://www.oecd-nea.org/tools/abstract/detail/NEA-1792
.. _NJOY: https://www.njoy21.io/NJOY2016/
.. _PREPRO: https://www-nds.iaea.org/ndspub/endf/prepro/
.. _PREPRO: https://www-nds.iaea.org/public/endf/prepro/
.. _ENDF-6 Format: https://www.oecd-nea.org/dbdata/data/manual-endf/endf102.pdf
.. _Monte Carlo Sampler: https://permalink.lanl.gov/object/tr?what=info:lanl-repo/lareport/LA-09721-MS
.. _Monte Carlo Sampler: https://mcnp.lanl.gov/pdf_files/TechReport_1983_LANL_LA-9721-MS_EverettCashwell.pdf
.. _LA-UR-14-27694: https://permalink.lanl.gov/object/tr?what=info:lanl-repo/lareport/LA-UR-14-27694
.. _LA-UR-14-27694: https://www.osti.gov/biblio/1159204
.. _MC21: https://www.osti.gov/biblio/903083
@ -1763,6 +1772,4 @@ types.
.. _Sutton and Brown: https://www.osti.gov/biblio/307911
.. _lectures: https://laws.lanl.gov/vhosts/mcnp.lanl.gov/pdf_files/la-ur-05-4983.pdf
.. _MCNP Manual: https://laws.lanl.gov/vhosts/mcnp.lanl.gov/pdf_files/la-ur-03-1987.pdf
.. _lectures: https://mcnp.lanl.gov/pdf_files/TechReport_2005_LANL_LA-UR-05-4983_Brown.pdf

View file

@ -609,17 +609,17 @@ is actually independent of the number of nodes:
.. _first paper: https://doi.org/10.2307/2280232
.. _work of Forrest Brown: http://hdl.handle.net/2027.42/24996
.. _work of Forrest Brown: https://deepblue.lib.umich.edu/handle/2027.42/24996
.. _Brissenden and Garlick: https://doi.org/10.1016/0306-4549(86)90095-2
.. _MPICH: http://www.mpich.org
.. _MPICH: https://www.mpich.org
.. _binomial tree: https://www.mcs.anl.gov/~thakur/papers/ijhpca-coll.pdf
.. _Geary: https://doi.org/10.2307/2342070
.. _Barnett: http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.51.7772
.. _Barnett: https://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.51.7772
.. _single-instruction multiple-data: https://en.wikipedia.org/wiki/SIMD

View file

@ -667,342 +667,6 @@ and Auger electrons:
5. Repeat from step 1 for vacancy left by the transition electron.
Electron-Positron Annihilation
------------------------------
When a positron collides with an electron, both particles are annihilated and
generally two photons with equal energy are created. If the kinetic energy of
the positron is high enough, the two photons can have different energies, and
the higher-energy photon is emitted preferentially in the direction of flight
of the positron. It is also possible to produce a single photon if the
interaction occurs with a bound electron, and in some cases three (or, rarely,
even more) photons can be emitted. However, the annihilation cross section is
largest for low-energy positrons, and as the positron energy decreases, the
angular distribution of the emitted photons becomes isotropic.
In OpenMC, we assume the most likely case in which a low-energy positron (which
has already lost most of its energy to bremsstrahlung radiation) interacts with
an electron which is free and at rest. Two photons with energy equal to the
electron rest mass energy :math:`m_e c^2 = 0.511` MeV are emitted isotropically
in opposite directions.
Bremsstrahlung
--------------
When a charged particle is decelerated in the field of an atom, some of its
kinetic energy is converted into electromagnetic radiation known as
bremsstrahlung, or 'braking radiation'. In each event, an electron or positron
with kinetic energy :math:`T` generates a photon with an energy :math:`E`
between :math:`0` and :math:`T`. Bremsstrahlung is described by a cross section
that is differential in photon energy, in the direction of the emitted photon,
and in the final direction of the charged particle. However, in Monte Carlo
simulations it is typical to integrate over the angular variables to obtain a
single differential cross section with respect to photon energy, which is often
expressed in the form
.. math::
:label: bremsstrahlung-dcs
\frac{d\sigma_{\text{br}}}{dE} = \frac{Z^2}{\beta^2} \frac{1}{E}
\chi(Z, T, \kappa),
where :math:`\kappa = E/T` is the reduced photon energy and :math:`\chi(Z, T,
\kappa)` is the scaled bremsstrahlung cross section, which is experimentally
measured.
Because electrons are attracted to atomic nuclei whereas positrons are
repulsed, the cross section for positrons is smaller, though it approaches that
of electrons in the high energy limit. To obtain the positron cross section, we
multiply :eq:`bremsstrahlung-dcs` by the :math:`\kappa`-independent factor used
in Salvat_,
.. math::
:label: positron-factor
\begin{aligned}
F_{\text{p}}(Z,T) =
& 1 - \text{exp}(-1.2359\times 10^{-1}t + 6.1274\times 10^{-2}t^2 - 3.1516\times 10^{-2}t^3 \\
& + 7.7446\times 10^{-3}t^4 - 1.0595\times 10^{-3}t^5 + 7.0568\times 10^{-5}t^6 \\
& - 1.8080\times 10^{-6}t^7),
\end{aligned}
where
.. math::
:label: positron-factor-t
t = \ln\left(1 + \frac{10^6}{Z^2}\frac{T}{\text{m}_\text{e}c^2} \right).
:math:`F_{\text{p}}(Z,T)` is the ratio of the radiative stopping powers for
positrons and electrons. Stopping power describes the average energy loss per
unit path length of a charged particle as it passes through matter:
.. math::
:label: stopping-power
-\frac{dT}{ds} = n \int E \frac{d\sigma}{dE} dE \equiv S(T),
where :math:`n` is the number density of the material and :math:`d\sigma/dE` is
the cross section differential in energy loss. The total stopping power
:math:`S(T)` can be separated into two components: the radiative stopping
power :math:`S_{\text{rad}}(T)`, which refers to energy loss due to
bremsstrahlung, and the collision stopping power :math:`S_{\text{col}}(T)`,
which refers to the energy loss due to inelastic collisions with bound
electrons in the material that result in ionization and excitation. The
radiative stopping power for electrons is given by
.. math::
:label: radiative-stopping-power
S_{\text{rad}}(T) = n \frac{Z^2}{\beta^2} T \int_0^1 \chi(Z,T,\kappa)
d\kappa.
To obtain the radiative stopping power for positrons,
:eq:`radiative-stopping-power` is multiplied by :eq:`positron-factor`.
While the models for photon interactions with matter described above can safely
assume interactions occur with free atoms, sampling the target atom based on
the macroscopic cross sections, molecular effects cannot necessarily be
disregarded for charged particle treatment. For compounds and mixtures, the
bremsstrahlung cross section is calculated using Bragg's additivity rule as
.. math::
:label: material-bremsstrahlung-dcs
\frac{d\sigma_{\text{br}}}{dE} = \frac{1}{\beta^2 E} \sum_i \gamma_i Z^2_i
\chi(Z_i, T, \kappa),
where the sum is over the constituent elements and :math:`\gamma_i` is the
atomic fraction of the :math:`i`-th element. Similarly, the radiative stopping
power is calculated using Bragg's additivity rule as
.. math::
:label: material-radiative-stopping-power
S_{\text{rad}}(T) = \sum_i w_i S_{\text{rad},i}(T),
where :math:`w_i` is the mass fraction of the :math:`i`-th element and
:math:`S_{\text{rad},i}(T)` is found for element :math:`i` using
:eq:`radiative-stopping-power`. The collision stopping power, however, is a
function of certain quantities such as the mean excitation energy :math:`I` and
the density effect correction :math:`\delta_F` that depend on molecular
properties. These quantities cannot simply be summed over constituent elements
in a compound, but should instead be calculated for the material. The Bethe
formula can be used to find the collision stopping power of the material:
.. math::
:label: material-collision-stopping-power
S_{\text{col}}(T) = \frac{2 \pi r_e^2 m_e c^2}{\beta^2} N_A \frac{Z}{A_M}
[\ln(T^2/I^2) + \ln(1 + \tau/2) + F(\tau) - \delta_F(T)],
where :math:`N_A` is Avogadro's number, :math:`A_M` is the molar mass,
:math:`\tau = T/m_e`, and :math:`F(\tau)` depends on the particle type. For
electrons,
.. math::
:label: F-electron
F_{-}(\tau) = (1 - \beta^2)[1 + \tau^2/8 - (2\tau + 1) \ln2],
while for positrons
.. math::
:label: F-positron
F_{+}(\tau) = 2\ln2 - (\beta^2/12)[23 + 14/(\tau + 2) + 10/(\tau + 2)^2 +
4/(\tau + 2)^3].
The density effect correction :math:`\delta_F` takes into account the reduction
of the collision stopping power due to the polarization of the material the
charged particle is passing through by the electric field of the particle.
It can be evaluated using the method described by Sternheimer_, where the
equation for :math:`\delta_F` is
.. math::
:label: density-effect-correction
\delta_F(\beta) = \sum_{i=1}^n f_i \ln[(l_i^2 + l^2)/l_i^2] -
l^2(1-\beta^2).
Here, :math:`f_i` is the oscillator strength of the :math:`i`-th transition,
given by :math:`f_i = n_i/Z`, where :math:`n_i` is the number of electrons in
the :math:`i`-th subshell. The frequency :math:`l` is the solution of the
equation
.. math::
:label: density-effect-l
\frac{1}{\beta^2} - 1 = \sum_{i=1}^{n} \frac{f_i}{\bar{\nu}_i^2 + l^2},
where :math:`\bar{v}_i` is defined as
.. math::
:label: density-effect-nubar
\bar{\nu}_i = h\nu_i \rho / h\nu_p.
The plasma energy :math:`h\nu_p` of the medium is given by
.. math::
:label: plasma-frequency
h\nu_p = \sqrt{\frac{(hc)^2 r_e \rho_m N_A Z}{\pi A}},
where :math:`A` is the atomic weight and :math:`\rho_m` is the density of the
material. In :eq:`density-effect-nubar`, :math:`h\nu_i` is the oscillator
energy, and :math:`\rho` is an adjustment factor introduced to give agreement
between the experimental values of the oscillator energies and the mean
excitation energy. The :math:`l_i` in :eq:`density-effect-correction` are
defined as
.. math::
:label: density-effect-li
\begin{aligned}
l_i &= (\bar{\nu}_i^2 + 2/3f_i)^{1/2} ~~~~&\text{for}~~ \bar{\nu}_i > 0 \\
l_n &= f_n^{1/2} ~~~~&\text{for}~~ \bar{\nu}_n = 0,
\end{aligned}
where the second case applies to conduction electrons. For a conductor,
:math:`f_n` is given by :math:`n_c/Z`, where :math:`n_c` is the effective
number of conduction electrons, and :math:`v_n = 0`. The adjustment factor
:math:`\rho` is determined using the equation for the mean excitation energy:
.. math::
:label: mean-excitation-energy
\ln I = \sum_{i=1}^{n-1} f_i \ln[(h\nu_i\rho)^2 + 2/3f_i(h\nu_p)^2]^{1/2} +
f_n \ln (h\nu_pf_n^{1/2}).
.. _ttb:
Thick-Target Bremsstrahlung Approximation
+++++++++++++++++++++++++++++++++++++++++
Since charged particles lose their energy on a much shorter distance scale than
neutral particles, not much error should be introduced by neglecting to
transport electrons. However, the bremsstrahlung emitted from high energy
electrons and positrons can travel far from the interaction site. Thus, even
without a full electron transport mode it is necessary to model bremsstrahlung.
We use a thick-target bremsstrahlung (TTB) approximation based on the models in
Salvat_ and Kaltiaisenaho_ for generating bremsstrahlung photons, which assumes
the charged particle loses all its energy in a single homogeneous material
region.
To model bremsstrahlung using the TTB approximation, we need to know the number
of photons emitted by the charged particle and the energy distribution of the
photons. These quantities can be calculated using the continuous slowing down
approximation (CSDA). The CSDA assumes charged particles lose energy
continuously along their trajectory with a rate of energy loss equal to the
total stopping power, ignoring fluctuations in the energy loss. The
approximation is useful for expressing average quantities that describe how
charged particles slow down in matter. For example, the CSDA range approximates
the average path length a charged particle travels as it slows to rest:
.. math::
:label: csda-range
R(T) = \int^T_0 \frac{dT'}{S(T')}.
Actual path lengths will fluctuate around :math:`R(T)`. The average number of
photons emitted per unit path length is given by the inverse bremsstrahlung
mean free path:
.. math::
:label: inverse-bremsstrahlung-mfp
\lambda_{\text{br}}^{-1}(T,E_{\text{cut}})
= n\int_{E_{\text{cut}}}^T\frac{d\sigma_{\text{br}}}{dE}dE
= n\frac{Z^2}{\beta^2}\int_{\kappa_{\text{cut}}}^1\frac{1}{\kappa}
\chi(Z,T,\kappa)d\kappa.
The lower limit of the integral in :eq:`inverse-bremsstrahlung-mfp` is non-zero
because the bremsstrahlung differential cross section diverges for small photon
energies but is finite for photon energies above some cutoff energy
:math:`E_{\text{cut}}`. The mean free path
:math:`\lambda_{\text{br}}^{-1}(T,E_{\text{cut}})` is used to calculate the
photon number yield, defined as the average number of photons emitted with
energy greater than :math:`E_{\text{cut}}` as the charged particle slows down
from energy :math:`T` to :math:`E_{\text{cut}}`. The photon number yield is
given by
.. math::
:label: photon-number-yield
Y(T,E_{\text{cut}}) = \int^{R(T)}_{R(E_{\text{cut}})}
\lambda_{\text{br}}^{-1}(T',E_{\text{cut}})ds = \int_{E_{\text{cut}}}^T
\frac{\lambda_{\text{br}}^{-1}(T',E_{\text{cut}})}{S(T')}dT'.
:math:`Y(T,E_{\text{cut}})` can be used to construct the energy spectrum of
bremsstrahlung photons: the number of photons created with energy between
:math:`E_1` and :math:`E_2` by a charged particle with initial kinetic energy
:math:`T` as it comes to rest is given by :math:`Y(T,E_1) - Y(T,E_2)`.
To simulate the emission of bremsstrahlung photons, the total stopping power
and bremsstrahlung differential cross section for positrons and electrons must
be calculated for a given material using :eq:`material-bremsstrahlung-dcs` and
:eq:`material-radiative-stopping-power`. These quantities are used to build the
tabulated bremsstrahlung energy PDF and CDF for that material for each incident
energy :math:`T_k` on the energy grid. The following algorithm is then applied
to sample the photon energies:
1. For an incident charged particle with energy :math:`T`, sample the number of
emitted photons as
.. math::
N = \lfloor Y(T,E_{\text{cut}}) + \xi_1 \rfloor.
2. Rather than interpolate the PDF between indices :math:`k` and :math:`k+1`
for which :math:`T_k < T < T_{k+1}`, which is computationally expensive, use
the composition method and sample from the PDF at either :math:`k` or
:math:`k+1`. Using linear interpolation on a logarithmic scale, the PDF can
be expressed as
.. math::
p_{\text{br}}(T,E) = \pi_k p_{\text{br}}(T_k,E) + \pi_{k+1}
p_{\text{br}}(T_{k+1},E),
where the interpolation weights are
.. math::
\pi_k = \frac{\ln T_{k+1} - \ln T}{\ln T_{k+1} - \ln T_k},~~~
\pi_{k+1} = \frac{\ln T - \ln T_k}{\ln T_{k+1} - \ln T_k}.
Sample either the index :math:`i = k` or :math:`i = k+1` according to the
point probabilities :math:`\pi_{k}` and :math:`\pi_{k+1}`.
3. Determine the maximum value of the CDF :math:`P_{\text{br,max}}`.
3. Sample the photon energies using the inverse transform method with the
tabulated CDF :math:`P_{\text{br}}(T_i, E)` i.e.,
.. math::
E = E_j \left[ (1 + a_j) \frac{\xi_2 P_{\text{br,max}} -
P_{\text{br}}(T_i, E_j)} {E_j p_{\text{br}}(T_i, E_j)} + 1
\right]^{\frac{1}{1 + a_j}}
where the interpolation factor :math:`a_j` is given by
.. math::
a_j = \frac{\ln p_{\text{br}}(T_i,E_{j+1}) - \ln p_{\text{br}}(T_i,E_j)}
{\ln E_{j+1} - \ln E_j}
and :math:`P_{\text{br}}(T_i, E_j) \le \xi_2 P_{\text{br,max}} \le
P_{\text{br}}(T_i, E_{j+1})`.
We ignore the range of the electron or positron, i.e., the bremsstrahlung
photons are produced in the same location that the charged particle was
created. The direction of the photons is assumed to be the same as the
direction of the incident charged particle, which is a reasonable approximation
at higher energies when the bremsstrahlung radiation is emitted at small
angles.
.. _photon_production:
@ -1059,16 +723,14 @@ emitted photon.
.. _anomalous scattering: http://pd.chem.ucl.ac.uk/pdnn/diff1/anomscat.htm
.. _Kahn's rejection method: https://laws.lanl.gov/vhosts/mcnp.lanl.gov/pdf_files/aecu-3259_kahn.pdf
.. _Kahn's rejection method: https://doi.org/10.2172/4353680
.. _Klein-Nishina: https://en.wikipedia.org/wiki/Klein%E2%80%93Nishina_formula
.. _LA-UR-04-0487: https://laws.lanl.gov/vhosts/mcnp.lanl.gov/pdf_files/la-ur-04-0487.pdf
.. _LA-UR-04-0487: https://mcnp.lanl.gov/pdf_files/TechReport_2004_LANL_LA-UR-04-0487_Sood.pdf
.. _LA-UR-04-0488: https://laws.lanl.gov/vhosts/mcnp.lanl.gov/pdf_files/la-ur-04-0488.pdf
.. _LA-UR-04-0488: https://mcnp.lanl.gov/pdf_files/TechReport_2004_LANL_LA-UR-04-0488_SoodWhite.pdf
.. _Kaltiaisenaho: https://aaltodoc.aalto.fi/bitstream/handle/123456789/21004/master_Kaltiaisenaho_Toni_2016.pdf
.. _Salvat: https://www.oecd-nea.org/globalsearch/download.php?doc=77434
.. _Sternheimer: https://doi.org/10.1103/PhysRevB.26.6067
.. _Salvat: https://doi.org/10.1787/32da5043-en

View file

@ -7,7 +7,7 @@ Random Number Generation
In order to sample probability distributions, one must be able to produce random
numbers. The standard technique to do this is to generate numbers on the
interval :math:`[0,1)` from a deterministic sequence that has properties that
make it appear to be random, e.g. being uniformly distributed and not exhibiting
make it appear to be random, e.g., being uniformly distributed and not exhibiting
correlation between successive terms. Since the numbers produced this way are
not truly "random" in a strict sense, they are typically referred to as
pseudorandom numbers, and the techniques used to generate them are pseudorandom
@ -15,6 +15,11 @@ number generators (PRNGs). Numbers sampled on the unit interval can then be
transformed for the purpose of sampling other continuous or discrete probability
distributions.
There are many different algorithms for pseudorandom number generation. OpenMC
currently uses `permuted congruential generator`_ (PCG), which builds on top of
the simpler linear congruential generator (LCG). Both algorithms are described
below.
------------------------------
Linear Congruential Generators
------------------------------
@ -37,8 +42,8 @@ be generated with a method chosen at random. Some theory should be used."
Typically, :math:`M` is chosen to be a power of two as this enables :math:`x
\mod M` to be performed using the bitwise AND operator with a bit mask. The
constants for the linear congruential generator used by default in OpenMC are
:math:`g = 2806196910506780709`, :math:`c = 1`, and :math:`M = 2^{63}` (see
`L'Ecuyer`_).
:math:`g = 2806196910506780709`, :math:`c = 1`, and :math:`M = 2^{63}` (from
`L'Ecuyer <https://doi.org/10.1090/S0025-5718-99-00996-5>`_).
Skip-ahead Capability
---------------------
@ -50,7 +55,8 @@ want to skip ahead :math:`N` random numbers and :math:`N` is large, the cost of
sampling :math:`N` random numbers to get to that position may be prohibitively
expensive. Fortunately, algorithms have been developed that allow us to skip
ahead in :math:`O(\log_2 N)` operations instead of :math:`O(N)`. One algorithm
to do so is described in a paper by Brown_. This algorithm relies on the following
to do so is described in a `paper by Brown
<https://www.osti.gov/biblio/976209>`_. This algorithm relies on the following
relationship:
.. math::
@ -58,15 +64,26 @@ relationship:
\xi_{i+k} = g^k \xi_i + c \frac{g^k - 1}{g - 1} \mod M
Note that equation :eq:`lcg-skipahead` has the same general form as equation :eq:`lcg`, so
the idea is to determine the new multiplicative and additive constants in
:math:`O(\log_2 N)` operations.
.. only:: html
.. rubric:: References
Note that equation :eq:`lcg-skipahead` has the same general form as equation
:eq:`lcg`, so the idea is to determine the new multiplicative and additive
constants in :math:`O(\log_2 N)` operations.
.. _L'Ecuyer: https://doi.org/10.1090/S0025-5718-99-00996-5
.. _Brown: https://laws.lanl.gov/vhosts/mcnp.lanl.gov/pdf_files/anl-rn-arb-stride.pdf
--------------------------------
Permuted Congruential Generators
--------------------------------
The `permuted congruential generator`_ (PCG) algorithm aims to improve upon the
LCG algorithm by permuting the output. The algorithm works on the basic
principle of first advancing the generator state using the LCG algorithm and
then applying a permutation function on the LCG state to obtain the output. This
results in increased statistical quality as measured by common statistical tests
while exhibiting a very small performance overhead relative to the LCG algorithm
and an equivalent memory footprint. For further details, see the original
technical report by `O'Neill
<https://www.pcg-random.org/pdf/hmc-cs-2014-0905.pdf>`_. OpenMC uses the
PCG-RXS-M-XS variant with a 64-bit state and 64-bit output.
.. _linear congruential generator: https://en.wikipedia.org/wiki/Linear_congruential_generator
.. _permuted congruential generator: https://en.wikipedia.org/wiki/Permuted_congruential_generator

File diff suppressed because it is too large Load diff

View file

@ -4,9 +4,9 @@
Tallies
=======
Note that the methods discussed in this section are written specifically for
continuous-energy mode but equivalent apply to the multi-group mode if the
particle's energy is replaced with the particle's group
The methods discussed in this section are written specifically for continuous-
energy mode. However, they can also apply to the multi-group mode if the
particle's energy is instead interpreted as the particle's group.
------------------
Filters and Scores
@ -205,7 +205,73 @@ had a collision at every event. Thus, for tallies with outgoing-energy filters
or for tallies of scattering moments (which require the scattering cosine of
the change-in-angle), we must use an analog estimator.
.. TODO: Add description of surface current tallies
-----------------------------------
Surface-Integrated Flux and Current
-----------------------------------
Surface tallies allow you to measure particle behavior as they cross specific
boundaries in your geometry. Unlike volume tallies, which integrate over a
volumetric region, surface tallies capture the current or flux passing through a
surface. Surface tallies are estimated using an analog estimator.
Current Score
-------------
When tallying the current across a surface, we simply count the weight of
particles that cross the surface of interest:
.. math::
:label: analog-current-estimator
J = \frac{1}{W} \sum_{i \in S} w_i.
where :math:`J` is the area-integrated current passing through surface
:math:`S`, :math:`W` is the total starting weight of the particles, and
:math:`w_i` is the weight of the particle as it crosses the surface :math:`S`.
Flux Score
----------
When tallying flux over a surface, we use the relationship between current and
flux:
.. math::
:label: surface-flux-estimator
\phi_S = \frac{1}{W} \sum_{i \in S} \frac{w_i}{|\mu|}.
where :math:`\phi_S` is the area-integrated flux over surface :math:`S`,
:math:`W` is the total starting weight of the particles, :math:`w_i` is the
weight of the particle as it crosses the surface :math:`S` and :math:`\mu` is
the cosine of angle between the particle direction and the surface normal.
This equation diverges when the particle crossing the surface is nearly parallel
to it (that is, as :math:`\mu` approaches zero). To remove this divergence,
OpenMC scores:
.. math::
:label: modified-surface-flux-estimator
\phi_S = \frac{1}{W} \sum_{i \in S} w_i f(\mu).
and the function :math:`f` is defined by:
.. math::
f(\mu) = \begin{cases}
\frac{1}{|\mu|} & |\mu| > \mu_\text{cut} \\
\frac{1}{c\mu_\text{cut}} & |\mu| \le \mu_\text{cut}
\end{cases}
where :math:`\mu_\text{cut}` is the grazing cosine cutoff and :math:`c` is the
cosine substitution ratio. The parameters :math:`\mu_\text{cut}` and :math:`c`
can be set by the user via the :attr:`openmc.Settings.surface_grazing_cutoff`
and :attr:`openmc.Settings.surface_grazing_ratio` attributes, respectively. The
default values for these parameters are 0.001 and 0.5 as recommended by
`Favorite, Thomas, and Booth <https://doi.org/10.13182/NSE09-72>`_.
.. _tallies_statistics:
----------
Statistics
@ -268,6 +334,14 @@ normal, log-normal, Weibull, etc. The central limit theorem states that as
Estimating Statistics of a Random Variable
------------------------------------------
After running OpenMC, each tallied quantity has a reported mean and standard
deviation. The below sections explain how these quantities are computed. Note
that OpenMC uses **batch statistics**, meaning that each observation for a tally
random variable corresponds to the aggregation of tally contributions from
multiple source particles that are grouped together into a single batch. See
:ref:`usersguide_particles` for more information on how the number of source
particles and statistical batches are specified.
Mean
++++
@ -377,6 +451,130 @@ of this is that the longer you run a simulation, the better you know your
results. Therefore, by running a simulation long enough, it is possible to
reduce the stochastic uncertainty to arbitrarily low levels.
Skewness
++++++++
The `skewness`_ of a population quantifies the asymmetry of the probability
distribution around its mean. Positive and negative skewness indicate a
longer/heavier right and left tail respectively. Let :math:`x_1,\ldots,x_n` be
the per-realization values for a bin, with sample mean :math:`\bar{x}` and
sample central moments:
.. math::
m_k \;=\; \frac{1}{n}\sum_{i=1}^{n}\bigl(x_i-\bar{x}\bigr)^k.
OpenMC reports the *adjusted Fisher-Pearson skewness* (defined for :math:`n \ge
3`), which is commonly used in many statistical packages:
.. math::
G_1 \;=\; \frac{\sqrt{n \cdot (n-1)}}{\,n-2\,}\cdot\frac{m_3}{m_2^{3/2}}.
where :math:`m_2` and :math:`m_3` correspond to the biased sample second and
third central moment respectively.
Kurtosis
++++++++
The `kurtosis`_ of a population quantifies tail weight (also called tailedness)
of the probability distribution relative to a normal distribution. Positive
excess kurtosis indicates *heavier tails* whereas negative excess kurtosis
indicates *lighter tails*. Kurtosis is especially useful for identifying bins
where occasional extreme scores dominate uncertainty. OpenMC reports the
*adjusted excess kurtosis* (defined for :math:`n \ge 4`):
.. math::
G_2 \;=\; \frac{(n-1)}{(n-2)(n-3)}
\left[(n+1)\,\frac{m_4}{m_2^{2}} \;-\; 3(n-1)\right].
where :math:`m_2` and :math:`m_4` correspond to the biased sample second and
fourth central moment respectively. For a perfectly normal distribution, the
excess kurtosis is :math:`0`.
Variance of Variance
++++++++++++++++++++
The variance of the variance (also known as the coefficient of variation
squared) measures *stability of the sample variance* :math:`s^2` and, by
extension, the reliability of reported relative errors. High VOV means that
error bars themselves are noisy—often due to heavy tails, skewness, or too few
realizations.
.. math::
VOV = \frac{s^2(s_{\bar{X}}^2)}{s_{\bar{X}}^4 } = \frac{m_4}{m_2^2} - \frac{1}{n}
where :math:`s_{\bar{X}}^2` is the estimated variance of the mean and
:math:`s^2(s_{\bar{X}}^2)` is the estimated variance in :math:`s_{\bar{X}}^2`.
The MCNP manual suggests a hard threshold such that :math:`VOV < 0.1` to improve
the probability of forming a reliable confidence interval. However, OpenMC does
not enforce an universal cut-off because the suitability of any single threshold
depends strongly on problem specifics (estimator choice, variance-reduction
settings, tally binning, or even effective sample size).
Normality Tests (D'Agostino-Pearson)
++++++++++++++++++++++++++++++++++++
These normality test verify the hypothesis that fluctuations are *approximately
normal*, a working assumption behind many Monte Carlo diagnostics and
`confidence-interval heuristics`_. Tests are provided for: (i) skewness-only,
(ii) kurtosis-only, and (iii) the *omnibus* combination. OpenMC uses the
finite-sample-adjusted skewness :math:`G_1` and excess kurtosis :math:`G_2`
above to construct standardized normal scores :math:`Z_1` (from :math:`G_1`) and
:math:`Z_2` (from :math:`G_2`) via the D'Agostino-Pearson transformations. The
omnibus statistic is
.. math::
K^2 \;=\; Z_1^{\,2} \;+\; Z_2^{\,2}
\;\sim\; \chi^2_{(2)} \quad \text{under } H_0:\ \text{normality}.
OpenMC reports :math:`Z_1`, :math:`Z_2`, :math:`K^2`, and their p-values when
prerequisites are met (skewness for :math:`n\ge 3`, kurtosis and omnibus for
:math:`n\ge 4`). Given a user-chosen significance level :math:`\alpha` (default
is :math:`0.05`), reject :math:`H_0` if :math:`\text{p-value}<\alpha`; otherwise
fail to reject. OpenMC leaves the interpretation to the user, who should
consider VOV together with skewness, kurtosis, and normality tests results when
judging whether reported confidence intervals are credible for their application
[#norm-tests]_.
.. [#norm-tests]
Higher-moments accumulation must be enabled with ``higher_moments = True``
for running these diagnostics including the skewness, kurtosis, and normality
tests.
Figure of Merit
+++++++++++++++
The figure of merit (FOM) is an indicator that accounts for both the statistical
uncertainty and the execution time and represents how much information is
obtained per unit time in the simulation. The FOM is defined as
.. math::
:label: figure_of_merit
FOM = \frac{1}{r^2 t},
where :math:`t` is the total execution time and :math:`r` is the relative error
defined as
.. math::
:label: relative_error
r = \frac{s_{\bar{X}}}{\bar{x}}.
Based on this definition, one can see that a higher FOM is desirable. The FOM is
useful as a comparative tool. For example, if a variance reduction technique is
being applied to a simulation, the FOM with variance reduction can be compared
to the FOM without variance reduction to ascertain whether the reduction in
variance outweighs the potential increase in execution time (e.g., due to
particle splitting). It is important to note that MCNP reports the FOM using CPU
time (wall-clock time multiplied by the number of threads/cores), whereas OpenMC
reports the FOM using only the wall-clock time :math:`t`.
Confidence Intervals
++++++++++++++++++++
@ -484,6 +682,8 @@ improve the estimate of the percentile.
.. rubric:: References
.. _confidence-interval heuristics: https://doi.org/10.1080/00031305.1990.10475751
.. _following approximation: https://doi.org/10.1080/03610918708812641
.. _Bessel's correction: https://en.wikipedia.org/wiki/Bessel's_correction
@ -504,6 +704,10 @@ improve the estimate of the percentile.
.. _converges in distribution: https://en.wikipedia.org/wiki/Convergence_of_random_variables#Convergence_in_distribution
.. _skewness: https://en.wikipedia.org/wiki/Skewness
.. _kurtosis: https://en.wikipedia.org/wiki/Kurtosis
.. _confidence intervals: https://en.wikipedia.org/wiki/Confidence_interval
.. _Student's t-distribution: https://en.wikipedia.org/wiki/Student%27s_t-distribution
@ -512,4 +716,4 @@ improve the estimate of the percentile.
.. _unpublished rational approximation: https://stackedboxes.org/2017/05/01/acklams-normal-quantile-function/
.. _MC21: http://www.osti.gov/bridge/servlets/purl/903083-HT5p1o/903083.pdf
.. _MC21: https://www.osti.gov/servlets/purl/903083

View file

@ -0,0 +1,216 @@
.. _methods_variance_reduction:
==================
Variance Reduction
==================
.. _methods_variance_reduction_intro:
------------
Introduction
------------
Transport problems can sometimes involve a significant degree of attenuation
between the source and a detector (tally) region, which can result in a flux
differential of ten orders of magnitude (or more) throughout the simulation
domain. As Monte Carlo uncertainties tend to be inversely proportional to the
physical flux density, it can be extremely difficult to accurately resolve
tallies in locations that are optically far from the source. This issue is
particularly common in fixed source simulations, where some tally locations may
not experience a single scoring event, even after billions of analog histories.
Variance reduction techniques aim to either flatten the global uncertainty
distribution, such that all regions of phase space have a fairly similar
uncertainty, or to reduce the uncertainty in specific locations (such as a
detector). There are three strategies available in OpenMC for variance
reduction: weight windows generated via the MAGIC method or the FW-CADIS method,
and source biasing. Both weight windowing strategies work by developing a mesh
that can be utilized by subsequent Monte Carlo solves to split particles heading
towards areas of lower flux densities while terminating particles in higher flux
regions. In contrast, source biasing modifies source site sampling behavior to
preferentially track particles more likely to reach phase space regions of
interest.
------------
MAGIC Method
------------
The Method of Automatic Generation of Importances by Calculation, or `MAGIC
method <https://doi.org/10.1016/j.fusengdes.2011.01.059>`_, is an iterative
technique that uses spatial flux information :math:`\phi(r)` obtained from a
normal Monte Carlo solve to produce weight windows :math:`w(r)` that can be
utilized by a subsequent iteration of Monte Carlo. While the first generation of
weight windows produced may only help to reduce variance slightly, use of these
weights to generate another set of weight windows results in a progressively
improving iterative scheme.
Equation :eq:`magic` defines how the lower bound of weight windows
:math:`w_{\ell}(r)` are generated with MAGIC using forward flux information.
Here, we can see that the flux at location :math:`r` is normalized by the
maximum flux in any group at that location. We can also see that the weights are
divided by a factor of two, which accounts for the typical :math:`5\times`
factor separating the lower and upper weight window bounds in OpenMC.
.. math::
:label: magic
w_{\ell}(r) = \frac{\phi(r)}{2\,\text{max}(\phi(r))}
A major advantage of this technique is that it does not require any special
transport machinery; it simply uses multiple Monte Carlo simulations to
iteratively improve a set of weight windows (which are typically defined on a
mesh covering the simulation domain). The downside to this method is that as the
flux differential increases between areas near and far from the source, it
requires more outer Monte Carlo iterations, each of which can be expensive in
itself. Additionally, computation of weight windows based on regular (forward)
neutron flux tally information does not produce the most numerically effective
set of weight windows. Nonetheless, MAGIC remains a simple and effective
technique for generating weight windows.
--------
FW-CADIS
--------
As discussed in the previous section, computation of weight windows based on
regular (forward) neutron flux tally information does not produce the most
numerically efficient set of weight windows. It is highly preferable to generate
weight windows based on spatial adjoint flux :math:`\phi^{\dag}(r)`
information. The adjoint flux is essentially the "reverse" simulation problem,
where we sample a random point and assume this is where a particle was absorbed,
and then trace it backwards (upscattering in energy), until we sample the point
where it was born from.
The Forward-Weighted Consistent Adjoint Driven Importance Sampling method, or
`FW-CADIS method <https://doi.org/10.13182/NSE12-33>`_, produces weight windows
for global or local variance reduction given adjoint flux information throughout
the entire domain. The weight window lower bound is defined in Equation
:eq:`fw_cadis`, and also involves a normalization step not shown here.
.. math::
:label: fw_cadis
w_{\ell}(r) = \frac{1}{2\phi^{\dag}(r)}
While the algorithm itself is quite simple, it requires estimates of the global
adjoint flux distribution, which is difficult to generate directly with Monte
Carlo transport. Thus, FW-CADIS typically uses an alternative solver (often
deterministic) that can be more readily adapted for generating adjoint flux
information, and which is often much cheaper than Monte Carlo given that a rough
solution is often sufficient for weight window generation.
The FW-CADIS implementation in OpenMC utilizes its own internal random ray
multigroup transport solver to generate the adjoint source distribution. No
coupling to any external transport is solver is necessary. The random ray solver
operates on the same geometry as the Monte Carlo solver, so no redefinition of
the simulation geometry is required. More details on how the adjoint flux is
computed are given in the :ref:`adjoint methods section <adjoint>`.
More information on the workflow is available in the :ref:`user guide
<variance_reduction>`, but generally production of weight windows with FW-CADIS
involves several stages (some of which are highly automated). These tasks
include generation of approximate multigroup cross section data for use by the
random ray solver, running of the random ray solver in normal (forward flux)
mode to generate a source for the adjoint solver, running of the random ray
solver in adjoint mode to generate adjoint flux tallies, and finally the
production of weight windows via the FW-CADIS method. As is discussed in the
user guide, most of these steps are automated together, making the additional
burden on the user fairly small.
The major advantage of this technique is that it typically produces much more
numerically efficient weight windows as compared to those generated with MAGIC,
sometimes with an order-of-magnitude improvement in the figure of merit
(Equation :eq:`variance_fom`), which accounts for both the variance and the
execution time. Another major advantage is that the cost of the random ray
solver is typically negligible compared to the cost of the subsequent Monte
Carlo solve itself, making it a very cheap method to deploy. The downside to
this method is that it introduces a second transport method into the mix (random
ray), such that there are more free input parameters for the user to know about
and adjust, potentially making the method more complex to use. However, as many
of the parameters have natural choices, much of this parameterization can be
handled automatically behind the scenes without the need for the user to be
aware of this.
.. math::
:label: variance_fom
\text{FOM} = \frac{1}{\text{Time} \times \sigma^2}
Finally, one unique capability of the FW-CADIS weight window generator is to
produce weight windows for local variance reduction, given a list of the
responses of interest. This is controlled by optionally specifying target
tallies from the :class:`openmc.model.Model` to the
:class:`openmc.WeightWindowGenerator`, as illustrated in the
:ref:`user guide<variance_reduction>`. If target tallies for local variance
reduction are supplied, then the adjoint sources are only populated after the
initial forward simulation in the source regions associated with those tallies.
In other regions, the adjoint source term is instead set to zero. The Random
Ray solver then determines the adjoint flux map used to generate FW-CADIS
weight windows following the usual technique.
.. _methods_source_biasing:
--------------
Source Biasing
--------------
In contrast to the previous two methods that introduce population controls
during transport, source biasing modifies the sampling of the external source
distribution. The basic premise of the technique is that for each spatial,
angular, energy, or time distribution of a source, an additional distribution
can be specified provided that the two share a common support (set of points
where the distribution is nonzero). Samples are then drawn from this "bias"
distribution, which can be chosen to preferentially direct particles towards
phase space regions of interest. In order to avoid biasing the tally results,
however, a weight adjustment is applied to each sampled site as described below.
Assume that the unbiased probability density function of a random variable
:math:`X:x \rightarrow \mathbb{R}` is given by :math:`f(x)`, but that using the
biased distribution :math:`g(x)` will result in a greater number of particle
trajectories reaching some phase space region of interest. Then a sample
:math:`x_0` may be drawn from :math:`g(x)` while maintaining a fair game,
provided that its weight is adjusted as:
.. math::
:label: source_bias
w = w_0 \times \frac{f(x_0)}{g(x_0)}
where :math:`w_0` is the weight of an unbiased sample from :math:`f(x)`,
typically unity.
Returning now to Equation :eq:`source_bias`, the requirement for common support
becomes evident. If :math:`\mathrm{supp} (g)` fully contains but is not
identical to :math:`\mathrm{supp} (f)`, then some samples from :math:`g(x)` will
correspond to points where :math:`f(x) = 0`. Thus these source sites would be
assigned a starting weight of 0, meaning the particles would be killed
immediately upon transport, effectively wasting computation time. Conversely, if
:math:`\mathrm{supp} (g)` is fully contained by but not identical to
:math:`\mathrm{supp} (f)`, the contributions of some regions outside
:math:`\mathrm{supp} (g)` will not be counted towards the integral, potentially
biasing the tally. The weight assigned to such points would be undefined since
:math:`g(x) = \mathbf{0}` at these points.
When an independent source is sampled in OpenMC, the particle's coordinate in
each variable of phase space :math:`(\mathbf{r},\mathbf{\Omega},E,t)` is
successively drawn from an independent probability distribution. Multiple
variables can be biased, in which case the resultant weight :math:`w` applied to
the particle is the product of the weights assigned from all sampled
distributions: space, angle, energy, and time, as shown in Equation
:eq:`tot_wgt`.
.. math::
:label: tot_wgt
w = w_r \times w_{\Omega} \times w_E \times w_t
Finally, source biasing and weight windows serve different purposes. Source
biasing changes how particles are born, allowing the initial source sites to be
sampled preferentially from important regions of phase space (space, angle,
energy, and time) with an accompanying weight adjustment. Weight windows, by
contrast, apply population control during transport (splitting and Russian
roulette) to help particles reach and contribute in important regions as they
move through the system. Because particle transport proceeds as usual after a
biased source is sampled, particle attenuation in optically thick regions
outside the source volume will not be affected by source biasing; in such
scenarios, transport biasing techniques such as weight windows are often more
effective.

View file

@ -138,8 +138,8 @@ Geometry and Visualization
*Trans. Am. Nucl. Soc.*, **114**, 391-394 (2016).
- Derek M. Lax, "`Memory efficient indexing algorithm for physical properties in
OpenMC <http://hdl.handle.net/1721.1/97862>`_," S. M. Thesis, Massachusetts
Institute of Technology (2015).
OpenMC <https://dspace.mit.edu/handle/1721.1/97862>`_," S. M. Thesis,
Massachusetts Institute of Technology (2015).
- Derek Lax, William Boyd, Nicholas Horelik, Benoit Forget, and Kord Smith, "A
memory efficient algorithm for classifying unique regions in constructive
@ -399,7 +399,8 @@ Doppler Broadening
- Jonathan A. Walsh, Benoit Forget, Kord S. Smith, Brian C. Kiedrowski, and
Forrest B. Brown, "`Direct, on-the-fly calculation of unresolved resonance
region cross sections in Monte Carlo simulations
<http://hdl.handle.net/1721.1/108644>`_," *Proc. Joint Int. Conf. M&C+SNA+MC*,
<https://dspace.mit.edu/handle/1721.1/108644>`_," *Proc. Joint Int. Conf.
M&C+SNA+MC*,
Nashville, Tennessee, Apr. 19--23 (2015).
- Colin Josey, Benoit Forget, and Kord Smith, "`Windowed multipole sensitivity
@ -596,7 +597,8 @@ Depletion
- Matthew S. Ellis, Colin Josey, Benoit Forget, and Kord Smith, "`Spatially
Continuous Depletion Algorithm for Monte Carlo Simulations
<http://hdl.handle.net/1721.1/107880>`_," *Trans. Am. Nucl. Soc.*, **115**,
<https://dspace.mit.edu/handle/1721.1/107880>`_," *Trans. Am. Nucl. Soc.*,
**115**,
1221-1224 (2016).
- Anas Gul, K. S. Chaudri, R. Khan, and M. Azeen, "`Development and verification

View file

@ -25,6 +25,8 @@ Simulation Settings
openmc.IndependentSource
openmc.FileSource
openmc.CompiledSource
openmc.MeshSource
openmc.TokamakSource
openmc.SourceParticle
openmc.VolumeCalculation
openmc.Settings
@ -34,8 +36,8 @@ Simulation Settings
:nosignatures:
:template: myfunction.rst
openmc.read_source_file
openmc.write_source_file
openmc.wwinp_to_wws
Material Specification
----------------------
@ -118,6 +120,7 @@ Constructing Tallies
openmc.Filter
openmc.UniverseFilter
openmc.MaterialFilter
openmc.MaterialFromFilter
openmc.CellFilter
openmc.CellFromFilter
openmc.CellBornFilter
@ -125,10 +128,14 @@ Constructing Tallies
openmc.CollisionFilter
openmc.SurfaceFilter
openmc.MeshFilter
openmc.MeshBornFilter
openmc.MeshMaterialFilter
openmc.MeshSurfaceFilter
openmc.EnergyFilter
openmc.EnergyoutFilter
openmc.ParticleProductionFilter
openmc.MuFilter
openmc.MuSurfaceFilter
openmc.PolarFilter
openmc.AzimuthalFilter
openmc.DistribcellFilter
@ -138,18 +145,31 @@ Constructing Tallies
openmc.SpatialLegendreFilter
openmc.SphericalHarmonicsFilter
openmc.TimeFilter
openmc.WeightFilter
openmc.ZernikeFilter
openmc.ZernikeRadialFilter
openmc.ParentNuclideFilter
openmc.ParticleFilter
openmc.ReactionFilter
openmc.MeshMaterialVolumes
openmc.Trigger
openmc.TallyDerivative
openmc.Tally
openmc.Tallies
Meshes
------
.. autosummary::
:toctree: generated
:nosignatures:
:template: myclassinherit.rst
openmc.RegularMesh
openmc.RectilinearMesh
openmc.CylindricalMesh
openmc.SphericalMesh
openmc.UnstructuredMesh
openmc.Trigger
openmc.TallyDerivative
openmc.Tally
openmc.Tallies
Geometry Plotting
-----------------
@ -159,8 +179,10 @@ Geometry Plotting
:nosignatures:
:template: myclass.rst
openmc.Plot
openmc.ProjectionPlot
openmc.SlicePlot
openmc.VoxelPlot
openmc.WireframeRayTracePlot
openmc.SolidRayTracePlot
openmc.Plots
Running OpenMC
@ -186,6 +208,7 @@ Post-processing
:template: myclass.rst
openmc.Particle
openmc.ParticleList
openmc.ParticleTrack
openmc.StatePoint
openmc.Summary
@ -197,6 +220,9 @@ Post-processing
:nosignatures:
:template: myfunction.rst
openmc.read_collision_track_file
openmc.read_collision_track_hdf5
openmc.read_collision_track_mcpl
openmc.voxel_to_vtk
The following classes and functions are used for functional expansion reconstruction.
@ -239,8 +265,16 @@ Variance Reduction
:template: myclass
openmc.WeightWindows
openmc.WeightWindowsList
openmc.WeightWindowGenerator
.. autosummary::
:toctree: generated
:nosignatures:
:template: myfunction.rst
openmc.hdf5_to_wws
openmc.wwinp_to_wws
Coarse Mesh Finite Difference Acceleration

View file

@ -16,15 +16,16 @@ Functions
current_batch
export_properties
export_weight_windows
import_weight_windows
finalize
find_cell
find_material
dagmc_universe_cell_ids
global_bounding_box
global_tallies
hard_reset
id_map
import_properties
import_weight_windows
init
is_statepoint_batch
iter_batches
@ -39,10 +40,12 @@ Functions
reset_timers
run
run_in_memory
run_random_ray
sample_external_source
simulation_init
simulation_finalize
simulation_init
source_bank
statepoint_load
statepoint_write
Classes
@ -53,12 +56,98 @@ Classes
:nosignatures:
:template: myclass.rst
AzimuthalFilter
Cell
CellFilter
CellInstanceFilter
CellbornFilter
CellfromFilter
CollisionFilter
CylindricalMesh
DelayedGroupFilter
DistribcellFilter
EnergyFilter
MaterialFilter
EnergyFunctionFilter
EnergyoutFilter
Filter
LegendreFilter
Material
MaterialFilter
MaterialFromFilter
Mesh
MeshFilter
MeshBornFilter
MeshSurfaceFilter
MuFilter
Nuclide
ParentNuclideFilter
ParticleFilter
ParticleProductionFilter
PolarFilter
ReactionFilter
RectilinearMesh
RegularMesh
SpatialLegendreFilter
SphericalHarmonicsFilter
SphericalMesh
SolidRayTracePlot
SurfaceFilter
Tally
TemporarySession
UniverseFilter
UnstructuredMesh
WeightFilter
WeightWindows
ZernikeFilter
ZernikeRadialFilter
Data
----
.. data:: cells
Mapping of cell ID to :class:`openmc.lib.Cell` instances.
:type: dict
.. data:: filters
Mapping of filter ID to :class:`openmc.lib.Filter` instances.
:type: dict
.. data:: materials
Mapping of material ID to :class:`openmc.lib.Material` instances.
:type: dict
.. data:: meshes
Mapping of mesh ID to :class:`openmc.lib.Mesh` instances.
:type: dict
.. data:: plots
Mapping of plot ID to :class:`openmc.lib.SolidRayTracePlot` instances.
:type: dict
.. data:: nuclides
Mapping of nuclide name to :class:`openmc.lib.Nuclide` instances.
:type: dict
.. data:: tallies
Mapping of tally ID to :class:`openmc.lib.Tally` instances.
:type: dict
.. data:: weight_windows
Mapping of weight window ID to :class:`openmc.lib.WeightWindows` instances.
:type: dict

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