Nuclear Level Density and the Determination of Thermonuclear Rates for Astrophysics

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dc.creatorRauscher, T.
dc.creatorThielemann, F. -K.
dc.creatorKratz, K. -L.
dc.date1997-06-30
dc.date.accessioned2026-07-07T11:08:24Z
dc.date.available2026-07-07T11:08:24Z
dc.descriptionThe prediction of cross sections for nuclei far off stability is crucial in the field of nuclear astrophysics. We discuss the model mostly employed for such calculations: the statistical model (Hauser-Feshbach). Special emphasis is put on the uncertainties arising from nuclear level density descriptions and an improved global description is presented. Furthermore, criteria for the applicability of the statistical model are investigated and a "map" for the applicability of the model to reactions of stable and unstable nuclei with neutral and charged particles is given.
dc.descriptionREVTeX paper + 7 B/W figures + 2 color figures; PRC, in press. Also available at http://quasar.physik.unibas.ch/preps.html
dc.identifierhttps://arxiv.org/abs/astro-ph/9706294
dc.identifierhttp://arxiv.org/abs/astro-ph/9706294
dc.identifierPhys.Rev.C56:1613-1625,1997
dc.identifierdoi:10.1103/PhysRevC.56.1613
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/190126
dc.subjectAstrophysics
dc.subjectNuclear Theory
dc.titleNuclear Level Density and the Determination of Thermonuclear Rates for Astrophysics
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