出版社：SISSA, Scuola Internazionale Superiore di Studi Avanzati
摘要：The "Karlsruhe Astrophysical Database of Nucleosynthesis in Stars" (KADoNiS) project is an
online database for experimental cross sections relevant to the s process and p process. It is
available under http://nuclear-astrophysics.fzk.de/kadonis and consists of two parts. Part 1 is an
updated sequel to the well-known Bao et al. compilations from 1987 and 2000, which is online
since April 2005. An extension of this s-process database to (n, p) and (n,a) cross sections at kT=
30 keV, as in the first version of the Bao compilation, is planned. The second part of KADoNiS
is a p-process library, which includes all available experimental data from (p,g ), (p,n), (a,g ),
(a,n), (a,a), (n,a) and (g ,n) reactions in or close to the respective Gamow window. Despite
the great number of reactions required for a p-process reaction network, experimental data is still
scarce and up to now restricted to stable targets. Given here is a short overview about the present
status of the KADoNiS database.
