TY - JOUR
T1 - Are there only 30 p nuclei?
AU - Dillmann, I.
AU - Käppeler, Franz
AU - Rauscher, Thomas
AU - Thielemann, F. K.
AU - Gallino, Roberto
AU - Bisterzo, Sara
PY - 2008
Y1 - 2008
N2 - We have performed p-process simulations with the most recent stellar (n,γ) cross sections from the "Karlsruhe Astrophysical Database of Nucleosynthesis in Stars" project (version v0.2, http://www.kadonis.org). The simulations were carried out with a parametrized supernova type II shock front model ("γ process") of a 25 solar mass star. The four isotopes 113In, 115Sn, 152Gd, and 164Er were not produced in these simulations, consistent with prior findings. Whereas for 152Gd and 164Er large s-process contributions were found, the origin of the observed solar 113In and 115Sn abundance is still under discussion.
AB - We have performed p-process simulations with the most recent stellar (n,γ) cross sections from the "Karlsruhe Astrophysical Database of Nucleosynthesis in Stars" project (version v0.2, http://www.kadonis.org). The simulations were carried out with a parametrized supernova type II shock front model ("γ process") of a 25 solar mass star. The four isotopes 113In, 115Sn, 152Gd, and 164Er were not produced in these simulations, consistent with prior findings. Whereas for 152Gd and 164Er large s-process contributions were found, the origin of the observed solar 113In and 115Sn abundance is still under discussion.
UR - http://www.scopus.com/inward/record.url?scp=84887269196&partnerID=8YFLogxK
M3 - Conference article
AN - SCOPUS:84887269196
SN - 1824-8039
JO - Proceedings of Science
JF - Proceedings of Science
T2 - 10th Symposium on Nuclei in the Cosmos, NIC 2008
Y2 - 27 July 2008 through 1 August 2008
ER -