Impacts of nuclear-physics uncertainties in the s-process determined by Monte-Carlo variations

Abstract

The s-process, a production mechanism based on slow-neutron capture during stellar evolution, is the origin of about half the elements heavier than iron. Abundance predictions for s-process nucleosynthesis depend strongly on the relevant neutron-capture and ${\hat{I}}^2$-decay rates, as well as on the details of the stellar model being considered. Here, we have used a Monte-Carlo approach to evaluate the nuclear uncertainty in s-process nucleosynthesis. We considered the helium burning of massive stars for the weak s-process and low-mass asymptotic-giant-branch stars for the main s-process. Our calculations include a realistic and general prescription for the temperature dependent uncertainty for the reaction cross sections. We find that the adopted uncertainty for ($\mathrm{n},{\hat{I}}^3$) rates, tens of per cent on average, effects the production of s-process nuclei along the line of ${\hat{I}}^2$-stability, and that the uncertainties in ${\hat{I}}^2$-decay from excited state contributions, has the strongest impact on branching points.

6 pages, 4 figures, 2 tables, the Proceedings of "the 2017 Symposium on Nuclear Data"; a supplementary article of arXiv:1701.00489