Evaluation of effective astrophysical S factor for non-resonant reactions.

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Campo Dublin Core	Valor	Idioma
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.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.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.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
Aparece nas coleções:	DECEA - Trabalhos apresentados em eventos

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