Isospin Effects on Astrophysical S-Factors

dc.creatorKimura, Sachie
dc.creatorBonasera, Aldo
dc.date2007-06-26
dc.date2007-11-13
dc.date.accessioned2026-07-07T10:36:13Z
dc.date.available2026-07-07T10:36:13Z
dc.descriptionWe estimate the ratios of bare astrophysical S-factors at zero incident energy for proton and deuteron induced reactions in a model which assumes a compound nucleus formation probability plus a statistical decay. The obtained ratios agree well with available experimental values, as far as the reactions which have dominant s-wave entrance channel components are investigated. Due to its simplicity the model could be used as a guidance for predictions on reactions which have not been investigated yet.
dc.description12 pages, 1 figures
dc.identifierhttps://arxiv.org/abs/0706.3864
dc.identifierhttp://arxiv.org/abs/0706.3864
dc.identifierPhys.Rev.C76:031602,2007
dc.identifierdoi:10.1103/PhysRevC.76.031602
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/179974
dc.subjectNuclear Theory
dc.titleIsospin Effects on Astrophysical S-Factors
dc.typetext

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