$p$-Process simulations with a modified reaction library

Details $p$-Process simulations with a modified reaction library $p$-Process simulations with a modified reaction library

2008-05-30

arxiv.org/abs/0805.4756v1

J.Phys.G35:014029,2008

Astronomy and Astrophysics

Astrophysics

5 pages, 1 figure Proceedings "Nuclear Physics in Astrophysics NPA-III", Dresden/Germany (2007)

Scientific paper

10.1088/0954-3899/35/1/014029

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 the Bi and Pb region around the $N$=126 shell closure.

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