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arXiv · 1507.03416

Nucleosynthesis simulations for the production of the p-nuclei $^{\text{92}}$Mo and $^{\text{94}}$Mo in a Supernova type II model

Kathrin Göbel·Jan Glorius·Alexander Koloczek·Marco Pignatari·René Reifarth·René Schach·Kerstin Sonnabend
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Abstract

We present a nucleosynthesis sensitivity study for the $\gamma$-process in a Supernova type II model within the NuGrid research platform. The simulations aimed at identifying the relevant local production and destruction rates for the p-nuclei of molybdenum and at determining the sensitivity of the final abundances to these rates. We show that local destruction rates strongly determine the abundance of $^{92}$Mo and $^{94}$Mo, and quantify the impact.

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Kathrin Göbel, Jan Glorius, Alexander Koloczek, Marco Pignatari, René Reifarth, René Schach, Kerstin Sonnabend. 2015-07-13. Nucleosynthesis simulations for the production of the p-nuclei $^{\text{92}}$Mo and $^{\text{94}}$Mo in a Supernova type II model. https://doi.org/10.1051/epjconf/20159303006

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