New Stellar $(n,γ)$ Cross Sections and The "Karlsruhe Astrophysical Database of Nucleosynthesis in Stars"

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dc.creatorDillmann, I.
dc.creatorPlag, R.
dc.creatorDomingo-Pardo, C.
dc.creatorHeil, M.
dc.creatorKäppeler, F.
dc.creatorRauscher, T.
dc.creatorThielemann, F. -K.
dc.date2008-06-12
dc.date.accessioned2026-07-07T09:44:12Z
dc.date.available2026-07-07T09:44:12Z
dc.descriptionSince April 2005 a regularly updated stellar neutron cross section compilation is available online at http://nuclear-astrophysics.fzk.de/kadonis. This online-database is called the "Karlsruhe Astrophysical Database of Nucleosynthesis in Stars" project and is based on the previous Bao et al. compilation from the year 2000. The present version \textsc{KADoNiS} v0.2 (January 2007) includes recommended cross sections for 280 isotopes between $^{1}$H and $^{210}$Po and 75 semi-empirical estimates for isotopes without experimental information. Concerning stellar $(n,γ)$ cross sections of the 32 stable, proton-rich isotopes produced by the $p$ process experimental information is only available for 20 isotopes, but 9 of them have rather large uncertainties of $\geq$9%. The first part of a systematic study of stellar $(n,γ)$ cross sections of the $p$-process isotopes $^{74}$Se, $^{84}$Sr, $^{102}$Pd, $^{120}$Te, $^{130}$Ba, $^{132}$Ba, $^{156}$Dy, and $^{174}$Hf is presented. In another application \textsc{KADoNiS} v0.2 was used for an modification of a reaction library of Basel university. With this modified library $p$-process network calculations were carried out and compared to previous results.
dc.descriptionProceedings "International Conference on Nuclear Data for Science and Technology 2007", Nice/ France
dc.identifierhttps://arxiv.org/abs/0806.2076
dc.identifierhttp://arxiv.org/abs/0806.2076
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/162789
dc.subjectAstrophysics
dc.subjectNuclear Experiment
dc.titleNew Stellar $(n,γ)$ Cross Sections and The "Karlsruhe Astrophysical Database of Nucleosynthesis in Stars"
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