Global Transmission Coefficients in Hauser-Feshbach Calculations for Astrophysics

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dc.creatorRauscher, T.
dc.date1998-02-09
dc.date.accessioned2026-07-07T05:42:17Z
dc.date.available2026-07-07T05:42:17Z
dc.descriptionThe current status of optical potentials employed in the prediction of thermonuclear reaction rates for astrophysics in the Hauser-Feshbach formalism is discussed. Special emphasis is put on $α$+nucleus potentials. A novel approach for the prediction of $α$+nucleus potentials is proposed. Further experimental efforts are motivated.
dc.description5 pages, LaTeX, to appear in "Hirschegg '98: Nuclear Astrophysics", Proc. Int. Workshop XXVI on Gross Properties of Nuclei and Nuclear Excitations, January 11-17, 1998, Hirschegg, Austria
dc.identifierhttps://arxiv.org/abs/nucl-th/9802026
dc.identifierhttp://arxiv.org/abs/nucl-th/9802026
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/82876
dc.subjectNuclear Theory
dc.subjectAstrophysics
dc.titleGlobal Transmission Coefficients in Hauser-Feshbach Calculations for Astrophysics
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