Abstract
Background: Precise understanding of nuclear fission is crucial for experimental and theoretical nuclear physics, astrophysics, and industrial applications; however, the complete physical mechanism is unresolved due to the complexities.
Purpose: In this study, we present a new method to describe the dynamical-fission process and following prompt-neutron emission, where we combine the dynamical fission calculation based on the Langevin method and the Hauser-Feshbach statistical model.
Methods: Two methods are connected smoothly within the universal charge distribution and the energy conservation, allowing us to calculate a sequence of fission dynamics and postfission phase, including prompt neutron emission.
Results: Using a certain set of model parameters, we successfully reproduce the experimental primary-fission yields, total kinetic energy, independent-fission yields, and prompt neutron emissions for the neutron-induced fission of , a compound nucleus of . We elucidate the physical mechanism of the characteristic features observed in previous experiments, such as shell properties. Additionally, we apply our calculation to two very neutron-rich uranium isotopes, i.e., and , which are not experimentally confirmed but are important for r-process nucleosynthesis. Theoretical results indicate that exhibits an asymmetric multiple-peak fission yield distribution, while the neutron-rich has a single peak due to symmetric fission. Our method predicts postneutron emission fragments, where shows a stronger neutron emissivity than .
Conclusions: Our framework is highly reproducible in the experiments and shows that the number of emitted neutrons after fission differs significantly in neutron-rich uranium fission depending on distributions of fission variables.
4 More- Received 17 July 2023
- Accepted 11 October 2023
DOI:https://doi.org/10.1103/PhysRevC.108.054607
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