Nucleosynthesis simulations for the production of the p-nuclei 92Mo and 94Mo in a Supernova type II model
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 a...
| Published in: | EPJ Web of Conferences |
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| Main Authors: | , , , , , , |
| Format: | Article |
| Language: | English |
| Published: |
EDP Sciences
2015-01-01
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| Online Access: | http://dx.doi.org/10.1051/epjconf/20159303006 |
| _version_ | 1852726649691308032 |
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| author | Göbel Kathrin Glorius Jan Koloczek Alexander Pignatari Marco Reifarth René Schach René Sonnabend Kerstin |
| author_facet | Göbel Kathrin Glorius Jan Koloczek Alexander Pignatari Marco Reifarth René Schach René Sonnabend Kerstin |
| author_sort | Göbel Kathrin |
| collection | DOAJ |
| container_title | EPJ Web of Conferences |
| description | 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 92Mo and 94Mo, and quantify the impact. |
| format | Article |
| id | doaj-art-d118eadebd5f4c2da1a8b4e7aaa1f49b |
| institution | Directory of Open Access Journals |
| issn | 2100-014X |
| language | English |
| publishDate | 2015-01-01 |
| publisher | EDP Sciences |
| record_format | Article |
| spelling | doaj-art-d118eadebd5f4c2da1a8b4e7aaa1f49b2025-08-19T21:10:17ZengEDP SciencesEPJ Web of Conferences2100-014X2015-01-01930300610.1051/epjconf/20159303006epjconf_cgs2015_03006Nucleosynthesis simulations for the production of the p-nuclei 92Mo and 94Mo in a Supernova type II modelGöbel KathrinGlorius JanKoloczek AlexanderPignatari MarcoReifarth RenéSchach RenéSonnabend Kerstin0Goethe University Frankfurt am MainWe 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 92Mo and 94Mo, and quantify the impact.http://dx.doi.org/10.1051/epjconf/20159303006 |
| spellingShingle | Göbel Kathrin Glorius Jan Koloczek Alexander Pignatari Marco Reifarth René Schach René Sonnabend Kerstin Nucleosynthesis simulations for the production of the p-nuclei 92Mo and 94Mo in a Supernova type II model |
| title | Nucleosynthesis simulations for the production of the p-nuclei 92Mo and 94Mo in a Supernova type II model |
| title_full | Nucleosynthesis simulations for the production of the p-nuclei 92Mo and 94Mo in a Supernova type II model |
| title_fullStr | Nucleosynthesis simulations for the production of the p-nuclei 92Mo and 94Mo in a Supernova type II model |
| title_full_unstemmed | Nucleosynthesis simulations for the production of the p-nuclei 92Mo and 94Mo in a Supernova type II model |
| title_short | Nucleosynthesis simulations for the production of the p-nuclei 92Mo and 94Mo in a Supernova type II model |
| title_sort | nucleosynthesis simulations for the production of the p nuclei 92mo and 94mo in a supernova type ii model |
| url | http://dx.doi.org/10.1051/epjconf/20159303006 |
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