Evaluation of effective astrophysical S factor for non-resonant reactions.
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2001
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We derived analytic formulas of the effective astrophysical S factor, Seff, for a non- resonant reaction of charged particles using a Taylor expansion of the astrophysical S factor, S(E), and a uniform approximation. The formulas will be able to generate more accurate approximations to Seff than previous ones.
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UEDA, M. et al. Evaluation of effective astrophysical S factor for non-resonant reactions. In: Proceedings of the 10th Yukawa International Seminar: YKIS01: Physics of Unstable Nuclei, 10., 2002, Kyoto. Anais… Kyoto: progress theoretical physics publication office, 2001. v. 146. p.634-635. Disponível em: <http://arxiv.org/pdf/nucl-th/0202040.pdf>. Acesso em: 27 set. 2012.