出版社：SISSA, Scuola Internazionale Superiore di Studi Avanzati
摘要：We have performed p-process simulations with the most recent stellar (n,g ) 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 (“g 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.
