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 abundances to these rates. We show that local destruction rates strongly determine the abundance of 92Mo and 94Mo, and quantify the impact.
Author: | Kathrin GöbelORCiDGND, Jan GloriusORCiDGND, Alexander KoloczekGND, Marco PignatariORCiD, René ReifarthORCiDGND, René Schach, Kerstin SonnabendGND |
---|---|
URN: | urn:nbn:de:hebis:30:3-719796 |
DOI: | https://doi.org/10.1051/epjconf/20159303006 |
ISSN: | 2100-014X |
Parent Title (English): | EPJ Web of Conferences |
Publisher: | EDP Sciences |
Place of publication: | Les Ulis |
Document Type: | Article |
Language: | English |
Date of Publication (online): | 2015/05/28 |
Date of first Publication: | 2015/05/28 |
Publishing Institution: | Universitätsbibliothek Johann Christian Senckenberg |
Contributing Corporation: | International Symposium on Capture Gamma-Ray Spectroscopy and Related Topics (15. : 2014 : Dresden) |
Release Date: | 2023/02/09 |
Volume: | 93 |
Issue: | 03006 |
Page Number: | 4 |
HeBIS-PPN: | 507202708 |
Institutes: | Physik / Physik |
Dewey Decimal Classification: | 5 Naturwissenschaften und Mathematik / 53 Physik / 530 Physik |
Sammlungen: | Universitätspublikationen |
Licence (German): | Creative Commons - Namensnennung 4.0 |