Angular Momentum of Fission Fragments from Microscopic Theory

TL;DR

This paper presents the first microscopic calculations of angular momentum distributions in fission fragments, revealing dependence on shell structure and deformation, and impacts on photon emission predictions.

Contribution

It introduces a microscopic approach to determine angular momentum distributions in fission fragments, linking them to nuclear structure and improving emission modeling.

Findings

Heavy fragments carry less angular momentum than light ones.

Angular momentum distributions influence photon emission counts.

Distributions follow a pattern consistent with experimental data.

Abstract

During nuclear fission, a heavy nucleus splits into two rotating fragments. The associated angular momentum is large, yet the mechanism of its generation and its dependence on the mass of fragments remain poorly understood. In this Letter, we provide the first microscopic calculations of angular momentum distributions in fission fragments for a wide range of fragment masses. For the benchmark case of $^{239}$Pu($n_{\text{th}}$,f), we find that the angular momentum of the fragments is largely determined by the nuclear shell structure and deformation, and that the heavy fragments therefore typically carry less angular momentum than their light partners. We use the fission model $\tt{FREYA}$ to simulate the emission of neutrons and photons from the fragments. The dependence of the angular momenta on fragment mass after the emission of neutrons and statistical photons is linear for the heavy fragments and either constant or weakly linear for the light fragments, consistent with the universal sawtooth pattern suggested by recent experimental data. Finally, we observe that using microscopic angular momentum distributions modifies the number of emitted photons significantly.