Evaluation of effective astrophysical S factor for non-resonant reactions.
dc.contributor.author | Ueda, Masahito | |
dc.contributor.author | Sargeant, Adam James | |
dc.contributor.author | Pato, Mauricio Porto | |
dc.contributor.author | Hussein, Mahir Saleh | |
dc.date.accessioned | 2012-09-27T13:23:53Z | |
dc.date.available | 2012-09-27T13:23:53Z | |
dc.date.issued | 2001 | |
dc.description.abstract | 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. | pt_BR |
dc.identifier.citation | 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. | pt_BR |
dc.identifier.uri | http://www.repositorio.ufop.br/handle/123456789/1450 | |
dc.language.iso | en_US | pt_BR |
dc.title | Evaluation of effective astrophysical S factor for non-resonant reactions. | pt_BR |
dc.type | Trabalho apresentado em evento | pt_BR |
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