Alpha clustering and the stellar nucleosynthesis of carbon

descriptionPublicationkeyboard_double_arrow_right Article , Part of book or chapter of book , Preprint , Other literature type 01 Sep 1994Embargo end date: 01 Jan 1993 English Publisher:Springer Science and Business Media LLCJournal:Zeitschrift f�r Physik A: Hadrons and Nuclei, volume 349, pages 241-242 (issn: 0939-7922, eissn: 1434-601X,

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Authors: Oberhummer, H.; Krauss, H.; Grün, K.; Rauscher, T.; Abele, H.; Mohr, P.; Staudt, G.;

doi: 10.1007/bf01288967 , 10.1007/978-3-642-79696-8_17 , 10.48550/arxiv.astro-ph/9310026 , 10.48550/arxiv.nucl-th/9310016

arXiv: astro-ph/9310026 , nucl-th/9310016

Alpha clustering and the stellar nucleosynthesis of carbon

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Abstract

The astrophysical S--factor and reaction rates for the triple--alpha process are calculated in the direct--capture model. It is shown that the stellar carbon production is extremely sensitive to small variations in the N--N interaction.

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Related Organizations

University of Tübingen
Germany
TU Wien
Austria

Keywords

Nuclear Theory (nucl-th), Nuclear Theory, Astrophysics (astro-ph), FOS: Physical sciences, Astrophysics

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