Isospin Effects on Astrophysical S-Factors
Nuclear Theory
2008-11-26 v2
Abstract
We 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.
Keywords
Cite
@article{arxiv.0706.3864,
title = {Isospin Effects on Astrophysical S-Factors},
author = {Sachie Kimura and Aldo Bonasera},
journal= {arXiv preprint arXiv:0706.3864},
year = {2008}
}