Revisiting the role of the $(n,\gamma f)$ process in the low-energy fission of $^{235}$U and $^{239}$Pu
J. Eric Lynn, Patrick Talou, Olivier Bouland

TL;DR
This paper reviews the $(n, ext{}\gamma f)$ process in low-energy fission of $^{235}$U and $^{239}$Pu, explaining observed fluctuations and the role of M1 transitions, with implications for nuclear reaction modeling.
Contribution
It provides a modern analysis of the $(n, ext{ }\gamma f)$ process, highlighting the significance of M1 transitions and low-lying modes in fission, extending understanding to fast neutron energies.
Findings
M1 transitions significantly contribute to pre-fission gamma spectra.
Fluctuations in neutron multiplicity and gamma energy are explained by transition state probabilities.
$(n, ext{ }\gamma f)$ corrections impact up to 3 ext% of total fission cross section.
Abstract
The process is reviewed in light of modern nuclear reaction calculations in both slow and fast neutron-induced fission reactions on U and Pu. Observed fluctuations of the average prompt fission neutron multiplicity and average total -ray energy below 100 eV incident neutron energy are interpreted in this framework. The surprisingly large contribution of the M1 transitions to the pre-fission -ray spectrum of Pu is explained by the dominant fission probabilities of 0 and transition states, which can only be accessed from compound nucleus states formed by the interaction of -wave neutrons with the target nucleus in its ground state, and decaying through M1 transitions. The impact of an additional low-lying M1 scissors mode in the photon strength function is analyzed. We review experimental evidence for fission fragment…
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