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Sensitivity study reveals diminished impact of fission on nuclear masses in r-process, highlighting its role in rare-earth peak formation.
A sensitivity study was performed to investigate the impact of individual nuclear masses on r-process rare-earth peak abundances in different astrophysical scenarios. The most impactful nuclei are primarily distributed in two regions on the nuclear chart: one located 20-30 neutrons away from stability (defined as region I ) and another 7-15 neutrons away from stability (defined as region II ), as previously reported in Phys. Lett. B 844, 138092 (2023). In this work, we extend our analysis focusing on the role of fission in the mass sensitivity study. The results show that in astrophysical scenarios involving fission, the sensitivity of nuclei in region I is diminished due to the deposition of a large number of fission fragments in the rare-earth mass region. However, nuclei in region II retain high sensitivity because the contribution of fission decreases in the later stages of nucleosynthesis. This study highlights the impact of fission on the sensitivity of r-process abundances to nuclear masses, and helps to enhance the understanding of the rare-earth peak formation mechanism.
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Hao et al. (2025) studied this question.
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