Present status of the KADoNiS database

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dc.creatorDillmann, I.
dc.creatorPlag, R.
dc.creatorHeil, M.
dc.creatorKäppeler, F.
dc.creatorRauscher, T.
dc.date2008-06-12
dc.date.accessioned2026-07-07T09:44:09Z
dc.date.available2026-07-07T09:44:09Z
dc.descriptionThe "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 $(n,α)$ 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 $(p,γ)$, $(p,n)$, $(α,γ)$, $(α,n)$, $(α,α)$, $(n,α)$ and $(γ,n)$ 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.
dc.descriptionProceedings "Nuclei in the Cosmos" NIC-IX, June 25-30 2006, CERN, Geneva/ Switzerland, published in "Proceedings of Science", PoS(NIC-IX)090
dc.identifierhttps://arxiv.org/abs/0806.2016
dc.identifierhttp://arxiv.org/abs/0806.2016
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/162769
dc.subjectAstrophysics
dc.subjectNuclear Experiment
dc.titlePresent status of the KADoNiS database
dc.typetext

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