http://arxiv.org/abs/1807.11475
Several thousand tracers from a 2D model of a thermonuclear supernova were used in a Monte Carlo post-processing approach to determine p-nuclide abundance uncertainties originating from nuclear physics uncertainties in the reaction rates.
T. Rauscher, N. Nishimura, R. Hirschi, et. al.
Wed, 1 Aug 18
54/65
Comments: 3 pages, 1 figure; to appear in Springer Proceedings of Physics as proceedings of the XV Int. Conf. “Nuclei in the Cosmos”, L’Aquila, Italy, June 2018. This conference contribution presents results published in MNRAS 474 (2018) 3133
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