Co-production of light and heavy $r$-process elements via fission deposition
Nicole Vassh, Matthew R. Mumpower, Gail C. McLaughlin, Trevor M., Sprouse, and Rebecca Surman

TL;DR
This paper introduces a self-consistent model for fission yields in r-process nucleosynthesis, showing how asymmetric fission contributes to the production of lighter heavy elements and supports the idea of universal abundance patterns in metal-poor stars.
Contribution
First application of macroscopic-microscopic fission yields in r-process simulations, linking fission fragment distributions to observed stellar abundance patterns.
Findings
Fission yields significantly influence light heavy element abundances.
Asymmetric fission contributes to palladium and silver production.
Results support the universality of r-process abundance patterns.
Abstract
We apply for the first time fission yields determined across the chart of nuclides from the macroscopic-microscopic theory of the Finite Range Liquid Drop Model to simulations of rapid neutron capture (-process) nucleosynthesis. With the fission rates and yields derived within the same theoretical framework utilized for other relevant nuclear data, our results represent an important step toward self-consistent applications of macroscopic-microscopic models in -process calculations. The yields from this model are wide for nuclei with extreme neutron excess. We show that these wide distributions of neutron-rich nuclei, and particularly the asymmetric yields for key species that fission at late times in the process, can contribute significantly to the abundances of the lighter heavy elements, specifically the light precious metals palladium and silver. Since these asymmetric…
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