p-Process simulations with a modified reaction library

Dillmann, I. and Rauscher, T. and Heil, M. and Kaeppeler, F. and Rapp, W. and Thielemann, F.-K.. (2008) p-Process simulations with a modified reaction library. Journal of physics. G, Nuclear and particle physics, Vol. 35, H. 1 , 14029, 5 S..

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Official URL: http://edoc.unibas.ch/dok/A5253878

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We have performed p-process simulations with the most recent stellar (n, gamma) cross sections from the Karlsruhe Astrophysical Database of Nucleosynthesis in Stars project (version v0.2, http://nuclear-astrophysics.fzk.de/kadonis). The simulations were carried out with a parametrized supernova type II shock front model (`gamma-process`) of a 25 solar mass star and compared to recently published results. A decrease in the normalized overproduction factor could be attributed to lower cross sections of a significant fraction of seed nuclei located in Bi and Pb regions around the N = 126 shell closure.
Faculties and Departments:05 Faculty of Science > Departement Physik > Former Organization Units Physics > Theoretische Physik Astrophysik (Thielemann)
UniBasel Contributors:Thielemann, Friedrich-Karl and Rauscher, Thomas
Item Type:Article, refereed
Article Subtype:Research Article
Publisher:IOP Publ.
Note:Publication type according to Uni Basel Research Database: Journal article
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Last Modified:22 Mar 2012 14:25
Deposited On:22 Mar 2012 13:46

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