Isospin Effects on Astrophysical S-Factors - Nuclear TheoryReport as inadecuate

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Abstract: We estimate the ratios of bare astrophysical S-factors at zero incidentenergy for proton and deuteron induced reactions in a model which assumes acompound nucleus formation probability plus a statistical decay. The obtainedratios agree well with available experimental values, as far as the reactionswhich have dominant s-wave entrance channel components are investigated. Due toits simplicity the model could be used as a guidance for predictions onreactions which have not been investigated yet.

Author: Sachie Kimura, Aldo Bonasera


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