# 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

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.