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.
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Acknowledgements
This work has been partially supported by the European Research Council (EU-FP7-ERC-2012-St Grant 306901), the EU COST Action CA16117 (ChETEC), the UK STFC (ST/M000958/1), and MEXT Japan (Priority Issue on Post-K computer: Elucidation of the Fundamental Laws and Evolution of the Universe). Parts of the computations were carried out on COSMOS (STFC DiRAC Facility) at the University of Cambridge. Further computations were carried out at CfCA, NAO Japan, and at YITP, Kyoto University.
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Rauscher, T., Nishimura, N., Hirschi, R., Murphy, A.S.J., Cescutti, G., Travaglio, C. (2019). Uncertainties in the Production of p Nuclides in SN Ia Determined by Monte Carlo Variations. In: Formicola, A., Junker, M., Gialanella, L., Imbriani, G. (eds) Nuclei in the Cosmos XV. Springer Proceedings in Physics, vol 219. Springer, Cham. https://doi.org/10.1007/978-3-030-13876-9_82
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