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arXiv · 2502.00599

Time Evolution of Prompt Gamma-Ray Emission in $^{252}$Cf(sf) and $^{233,235}$U($n$,f) Reactions

Patrick Talou·Amy E. Lovell·Ionel Stetcu·Gencho Rusev·Toshihiko Kawano·Marian Jandel
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Abstract

We investigate the time evolution of prompt fission $\gamma$ emission due to the presence of ns to ms isomers in the fragments produced in the neutron-induced fission of $^{233,235}$U and in the spontaneous fission of $^{252}$Cf. Calculations performed with the CGMF fission event generator are compared with recent experimental data on $^{252}$Cf(sf) and $^{235}$U($n$,f) obtained with the DANCE+NEUANCE setup at the Los Alamos Neutron Science Center. Of particular interest are the average $\gamma$-ray energy spectrum as a function of time since scission, $\phi(\epsilon_\gamma,t)$, the increase of the average $\gamma$-ray multiplicity over time, $N_\gamma(t)$, and its evolution in time as a function of the fission fragment mass, $N_\gamma(A,t)$. The time evolution of isomeric ratios in post-neutron emission fission fragments can be defined and used to test and reveal some deficiencies in our knowledge of the low-lying levels of neutron-rich nuclei produced in fission reactions.

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Patrick Talou, Amy E. Lovell, Ionel Stetcu, Gencho Rusev, Toshihiko Kawano, Marian Jandel. 2025-02-01. Time Evolution of Prompt Gamma-Ray Emission in $^{252}$Cf(sf) and $^{233,235}$U($n$,f) Reactions. https://arxiv.org/abs/2502.00599

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