OpenMC/docs/source/io_formats/data_wmp.rst

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.. _io_data_wmp:
=================================
Windowed Multipole Library Format
=================================
**/**
:Attributes: - **filetype** (*char[]*) -- String indicating the type of file
- **version** (*int[2]*) -- Major and minor version of the data
**/<nuclide name>/**
:Datasets:
- **broaden_poly** (*int[]*)
If 1, Doppler broaden curve fit for window with corresponding index.
If 0, do not.
- **curvefit** (*double[][][]*)
Curve fit coefficients. Indexed by (window index, coefficient index,
reaction type).
- **data** (*complex[][]*)
Complex poles and residues. Each pole has a corresponding set of
residues. For example, the :math:`i`-th pole and corresponding residues
are stored as
.. math::
\text{data}[:,i] = [\text{pole},~\text{residue}_1,~\text{residue}_2,
~\ldots]
The residues are in the order: scattering, absorption, fission. Complex
numbers are stored by forming a type with ":math:`r`" and ":math:`i`"
identifiers, similar to how `h5py`_ does it.
- **E_max** (*double*)
Highest energy the windowed multipole part of the library is valid for.
- **E_min** (*double*)
Lowest energy the windowed multipole part of the library is valid for.
- **spacing** (*double*)
.. math::
\frac{\sqrt{E_{max}} - \sqrt{E_{min}}}{n_w}
Where :math:`E_{max}` is the maximum energy the windows go up to.
:math:`E_{min}` is the minimum energy, and :math:`n_w` is the number of
windows, given by ``windows``.
- **sqrtAWR** (*double*)
Square root of the atomic weight ratio.
- **windows** (*int[][]*)
The poles to start from and end at for each window. windows[i, 0] and
windows[i, 1] are, respectively, the indexes (1-based) of the first and
last pole in window i.
.. _h5py: https://docs.h5py.org/en/latest/