[Submitted on 2 Aug 2017] (cross-list from astro-ph.SR)
The s-process nucleosynthesis: impact of the uncertainties in the nuclear physics determined by Monte Carlo variations
G. Cescutti · N. Nishimura · R. Hirschi · T. Rauscher · J. W. den Hartogh · A. St. J. Murphy
We investigated the impact of uncertainties in neutron-capture and weak reactions (on heavy elements) on the s-process nucleosynthesis in low-mass stars and massive stars using a Monte-Carlo based approach. We performed extensive nuclear reaction network calculations that include newly evaluated temperature-dependent upper and lower limits for the individual reaction rates. We found beta-decay rate uncertainties affect only a few nuclei near s-process branchings, whereas most of the uncertainty in the final abundances is caused by uncertainties in the neutron capture rates. We suggest a list of uncertain rates as candidates for improved measurement by future experiments.
- Comments:
- Proceedings of the conference "The AGB-Supernovae Mass Transition", held at Rome Observatory, March 27-31, 2017; in press for the Mem. Societa Astronomica Italiana (4 pages, 2 figures, and 1 table). arXiv admin note: text overlap with arXiv:1701.06978
- Subjects:
- Solar and Stellar Astrophysics (astro-ph.SR); Nuclear Experiment (nucl-ex); Nuclear Theory (nucl-th)
- arXiv:
- 1708.01629 [pdf]