Constraining astrophysical reaction rates: using the storage rings at FAIR/GSI
Ion optical calculations for a storage ring at the present GSI facility for direct proton-induced reactions relevant for different astrophysical processes are presented. As an example case, the 59Cu(p,γ) and 59Cu(p,α) reactions are shown. The branching of these two reactions is important in X-ray bu...
Main Authors: | , , , , , |
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Format: | Article |
Language: | English |
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EDP Sciences
2017-01-01
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Series: | EPJ Web of Conferences |
Online Access: | https://doi.org/10.1051/epjconf/201716501033 |
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author | Langer Christoph Glorius Jan Slavkovská Zuzana Litvinov Sergey Litvinov Yuri A. Reifarth René |
author_facet | Langer Christoph Glorius Jan Slavkovská Zuzana Litvinov Sergey Litvinov Yuri A. Reifarth René |
author_sort | Langer Christoph |
collection | DOAJ |
description | Ion optical calculations for a storage ring at the present GSI facility for direct proton-induced reactions relevant for different astrophysical processes are presented. As an example case, the 59Cu(p,γ) and 59Cu(p,α) reactions are shown. The branching of these two reactions is important in X-ray burst scenarios, since it determines the breakout out of the major 56Ni waiting point. |
first_indexed | 2024-12-16T11:47:10Z |
format | Article |
id | doaj.art-9284b54ae95b41f599ae1f0e6372fe4b |
institution | Directory Open Access Journal |
issn | 2100-014X |
language | English |
last_indexed | 2024-12-16T11:47:10Z |
publishDate | 2017-01-01 |
publisher | EDP Sciences |
record_format | Article |
series | EPJ Web of Conferences |
spelling | doaj.art-9284b54ae95b41f599ae1f0e6372fe4b2022-12-21T22:32:49ZengEDP SciencesEPJ Web of Conferences2100-014X2017-01-011650103310.1051/epjconf/201716501033epjconf_npa82017_01033Constraining astrophysical reaction rates: using the storage rings at FAIR/GSILanger ChristophGlorius JanSlavkovská ZuzanaLitvinov SergeyLitvinov Yuri A.Reifarth RenéIon optical calculations for a storage ring at the present GSI facility for direct proton-induced reactions relevant for different astrophysical processes are presented. As an example case, the 59Cu(p,γ) and 59Cu(p,α) reactions are shown. The branching of these two reactions is important in X-ray burst scenarios, since it determines the breakout out of the major 56Ni waiting point.https://doi.org/10.1051/epjconf/201716501033 |
spellingShingle | Langer Christoph Glorius Jan Slavkovská Zuzana Litvinov Sergey Litvinov Yuri A. Reifarth René Constraining astrophysical reaction rates: using the storage rings at FAIR/GSI EPJ Web of Conferences |
title | Constraining astrophysical reaction rates: using the storage rings at FAIR/GSI |
title_full | Constraining astrophysical reaction rates: using the storage rings at FAIR/GSI |
title_fullStr | Constraining astrophysical reaction rates: using the storage rings at FAIR/GSI |
title_full_unstemmed | Constraining astrophysical reaction rates: using the storage rings at FAIR/GSI |
title_short | Constraining astrophysical reaction rates: using the storage rings at FAIR/GSI |
title_sort | constraining astrophysical reaction rates using the storage rings at fair gsi |
url | https://doi.org/10.1051/epjconf/201716501033 |
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