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Hydrostatic and explosive nucleosynthesis in massive stars using improved nuclear and stellar physics

Rauscher, T. and Heger, A. and Hoffman, R. D. and Woosley, S. E.. (2003) Hydrostatic and explosive nucleosynthesis in massive stars using improved nuclear and stellar physics. Nuclear physics. A, Nuclear and hadronic physics, Vol. 718 , S. 463C-465C.

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Official URL: http://edoc.unibas.ch/dok/A5839281

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Abstract

We have performed the first calculations to follow the evolution of all stable nuclei and their radioactive progenitors in a finely-zoned stellar model computed from the onset of central hydrogen burning through explosion as a Type 11 supernova. Calculations were done for 15 M-circle dot, 19 M-circle dot, 20 Mcircle dot, 21 Mcircle dot, and 25 Mcircle dot Pop I stars using the most recently available set of experimental and theoretical nuclear data, revised opacity tables, and taking into account mass loss due to stellar winds. Here, we focus on the nuclear inputs.
Faculties and Departments:05 Faculty of Science > Departement Physik > Physik > Theoretische Physik Astrophysik (Thielemann)
UniBasel Contributors:Rauscher, Thomas
Item Type:Article, refereed
Article Subtype:Research Article
Bibsysno:Link to catalogue
Publisher:North Holland
ISSN:0375-9474
Note:Publication type according to Uni Basel Research Database: Journal article
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Last Modified:14 Sep 2012 07:18
Deposited On:14 Sep 2012 06:44

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