Impact of Nuclear Reaction Uncertainties on AGB Nucleosynthesis Models
Impact of Nuclear Reaction Uncertainties on AGB Nucleosynthesis Models
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Author / Creator
Bisterzo, S , Gallino, R , Kaeppeler, F , Wiescher, M and Travaglio, C
Publisher
Ithaca: Cornell University Library, arXiv.org
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Language
English
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Ithaca: Cornell University Library, arXiv.org
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Contents
Asymptotic giant branch (AGB) stars with low initial mass (1 - 3 Msun) are responsible for the production of neutron-capture elements through the main s-process (main slow neutron capture process). The major neutron source is 13C(alpha, n)16O, which burns radiatively during the interpulse periods at about 8 keV and produces a rather low neutron den...
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Full title
Impact of Nuclear Reaction Uncertainties on AGB Nucleosynthesis Models
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TN_cdi_proquest_journals_2086660752
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2086660752
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E-ISSN
2331-8422
DOI
10.48550/arxiv.1211.4970
