diff --git a/docs/source/usersguide/depletion.rst b/docs/source/usersguide/depletion.rst index e8dc21bca7..2d03e167b0 100644 --- a/docs/source/usersguide/depletion.rst +++ b/docs/source/usersguide/depletion.rst @@ -319,16 +319,18 @@ normalizing reaction rates: .. math:: - \phi = \frac{P}{V \cdot \sum\limits_i (Q_i \cdot \sigma^f_i \cdot n_i)} + \phi = \frac{P}{\sum\limits_i (Q_i \sigma^f_i n_i)} - where :math:`\sum_i` is the sum over all nuclides :math:`i`. This equation - makes the same assumptions and issues as discussed in - :ref:`energy-deposition`. Unfortunately, the proposed solution in that + where :math:`P` is the power, :math:`Q_i` is the fission Q value for nuclide + :math:`i`, :math:`\sigma_i^f` is the microscopic fission cross section for + nuclide :math:`i`, and :math:`N_i` is the number of atoms of nuclide + :math:`i`. This equation makes the same assumptions and issues as discussed + in :ref:`energy-deposition`. Unfortunately, the proposed solution in that section does not apply here since we are decoupled from transport code. However, there is a method to converge to a more accurate value for flux by - using substeps during time integration. - `This paper `_ provides a - good discussion of this method. + using substeps during time integration. `This paper + `_ provides a good discussion + of this method. .. warning::