Avoid negative heating values during pair production and bremsstrahlung (#3426)

Co-authored-by: GuySten <guyste@post.bgu.ac.il>
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Paul Romano 2025-06-05 10:45:49 -05:00 committed by GitHub
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@ -47,15 +47,17 @@ interactions, the energy-balance KERMA coefficient is
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 :math:`Q` value is zero and thus
the KERMA coefficient is
photon and charged particle interactions the KERMA coefficient is
.. math::
:label: energy-balance-photon
k_{i, r}(E) = \left(E - \sum\limits_x \bar{E}_{i, r, x}
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.
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Fission
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