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Nucleosynthesis simulations for the production of the p-nuclei 92Mo and 94Mo in a Supernova type II model

Göbel, Kathrin; Glorius, Jan; Koloczek, Alexander; Pignatari, Marco; Reifarth, René; Schach, René; Sonnabend, Kerstin

Authors

Kathrin Göbel

Jan Glorius

Alexander Koloczek

Marco Pignatari

René Reifarth

René Schach

Kerstin Sonnabend



Contributors

R. Schwengner
Editor

K. Zuber
Editor

Abstract

We present a nucleosynthesis sensitivity study for the γ-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.

Citation

Göbel, K., Glorius, J., Koloczek, A., Pignatari, M., Reifarth, R., Schach, R., & Sonnabend, K. (2015). Nucleosynthesis simulations for the production of the p-nuclei 92Mo and 94Mo in a Supernova type II model. EPJ Web of Conferences, 93, 03006. https://doi.org/10.1051/epjconf/20159303006

Journal Article Type Article
Online Publication Date May 28, 2015
Publication Date May 28, 2015
Deposit Date Jun 28, 2018
Publicly Available Date Jul 13, 2018
Journal EPJ Web of Conferences
Print ISSN 2100-014X
Electronic ISSN 2100-014X
Publisher EDP Sciences
Peer Reviewed Peer Reviewed
Volume 93
Article Number 03006
Pages 03006
ISBN 9782759817948
DOI https://doi.org/10.1051/epjconf/20159303006
Public URL https://hull-repository.worktribe.com/output/558411
Publisher URL https://www.epj-conferences.org/articles/epjconf/abs/2015/12/epjconf_cgs2015_03006/epjconf_cgs2015_03006.html

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Copyright Statement
© Owned by the authors, published by EDP Sciences, 2015. This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.





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