Hauser-Feshbach fission fragment de-excitation with calculated macroscopic-microscopic mass yields
The Hauser-Feshbach statistical model is applied to the de-excitation of primary fission fragments using input mass yields calculated with macroscopic-microscopic models of the potential energy surface. We test the sensitivity of the prompt fission observables to the input mass yields for two important reactions, $^{235}$U$(n_\mathrm{th},f)$ and $^{239}$Pu$(n_\mathrm{th},f)$, for which good experimental data exist. General traits of the mass yields, such as the location of the peaks and their widths, can impact both the prompt neutron and $γ$-ray multiplicities, as well as their spectra. Specifically, we use several mass yields to determine a linear correlation between the calculated prompt neutron multiplicity $\barν$ and the average heavy-fragment mass $\langle A_h\rangle$ of the input mass yields $\partial\barν/\partial\langle A_h\rangle = \pm 0.1\,n/f/\mathrm{u}$. The mass peak width influences the correlation between the total kinetic energy of the fission fragments and the total number of prompt neutrons emitted $\barν_T(\mathrm{TKE})$. Typical biases on prompt particle observables from using calculated mass yields instead of experimental ones are: $δ\barν = 4\%$ for the average prompt neutron multiplicity, $δ\bar{M}_γ= 1\%$ for the average prompt $γ$-ray multiplicity, $δ\barε_n^\mathrm{LAB} = 1\%$ for the average outgoing neutron energy, $δ\barε_γ= 1\%$ for the average $γ$-ray energy, and $δ\langle\mathrm{TKE}\rangle = 0.4\%$ for the average total kinetic energy of the fission fragments.