Uncertainties in the production of p nuclides in SN Ia determined by Monte Carlo variations
arXiv:1807.11475 · doi:10.1007/978-3-030-13876-9_82
Abstract
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.
arXiv comment3 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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