The fission
product yields were retrieved from the corresponding evaluated nuclear
data files using the AVRFPY code. They are usually given
on a very coarse energy grid (no more than three points), therefore it
is not necessary to use an elaborate weighting function for averaging.
A four points averaging function was defined in the AVRFPY code according
to the following conditions:
1. The lower
boundary of the thermal group is at 0.00001 eV or at the first energy
point at which the yields are given (whichever is higher).The upper boundary
of the thermal group is at 0.55 eV, which is approximately the cadmium
cutoff energy. The upper boundary of the epithermal group is at 1 keV.
The upper boundary of the fast group is 10 MeV.
2. The integral of the thermal spectrum is defined such that the spectral
ratio (i.e. ratio of the thermal flux to the sum of the epithermal and
fast flux) is 5.785.The integral of the fast spectrum is defined such
that the ratio of the fast to epithermal flux is 0.9279.
3. The fission cross section of the parent fissile nuclide is defined
in the same group structure from the average thermal cross section, the
resonance integral and the fission spectrum averaged cross section. The
fission reaction rate in three groups is calculated to define the weighting
function.
4. The spectrum at 0.55 eV is defined assuming 1/E shape in the epithermal
range. The fission cross section at this energy is defined assuming a
1/v cross section behavior in the thermal group, where v is the neutron
velocity. The reaction rate weighting function is the product of the spectrum
and the fission cross section. At other energies it is defined to conserve
the integrals, assuming log-log interpolation.
The three-group averaging flux is typical of light water reactors and
corresponds to the EPRI-CELL LWR spectrum available for cross section
averaging as option IWT=5 in the NJOY nuclear data processing system.
The fission reaction rate weighting function provides a unique and consistent
way of averaging the fission product yields. In practice, for common fissile
nuclides the contribution to the yields from the fast neutrons is only about
1% to 2 %, which hardly affects the interpolated yields. For fertile nuclides
with a fission threshold the yields consist almost entirely from the fast
contribution. |