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

Detalhes bibliográficos
Autor(a) principal: Ueda, Masahito
Data de Publicação: 2001
Outros Autores: Sargeant, Adam James, Pato, Mauricio Porto, Hussein, Mahir Saleh
Tipo de documento: Artigo de conferência
Idioma: eng
Título da fonte: Repositório Institucional da UFOP
Texto Completo: http://www.repositorio.ufop.br/handle/123456789/1450
Resumo: 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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spelling Ueda, MasahitoSargeant, Adam JamesPato, Mauricio PortoHussein, Mahir Saleh2012-09-27T13:23:53Z2012-09-27T13:23:53Z2001UEDA, 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.http://www.repositorio.ufop.br/handle/123456789/1450We 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.Evaluation of effective astrophysical S factor for non-resonant reactions.info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/conferenceObjectengreponame:Repositório Institucional da UFOPinstname:Universidade Federal de Ouro Preto (UFOP)instacron:UFOPinfo:eu-repo/semantics/openAccessLICENSElicense.txtlicense.txttext/plain; charset=utf-81748http://www.repositorio.ufop.br/bitstream/123456789/1450/5/license.txt8a4605be74aa9ea9d79846c1fba20a33MD55ORIGINALEVENTO_EvaluationEffectiveAstrophysical.pdfEVENTO_EvaluationEffectiveAstrophysical.pdfapplication/pdf73050http://www.repositorio.ufop.br/bitstream/123456789/1450/1/EVENTO_EvaluationEffectiveAstrophysical.pdf8bddaa2cd878dcdd2a81d7ad5abde4f9MD51123456789/14502019-03-11 10:09:35.852oai:localhost: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Repositório InstitucionalPUBhttp://www.repositorio.ufop.br/oai/requestrepositorio@ufop.edu.bropendoar:32332019-03-11T14:09:35Repositório Institucional da UFOP - Universidade Federal de Ouro Preto (UFOP)false
dc.title.pt_BR.fl_str_mv Evaluation of effective astrophysical S factor for non-resonant reactions.
title Evaluation of effective astrophysical S factor for non-resonant reactions.
spellingShingle Evaluation of effective astrophysical S factor for non-resonant reactions.
Ueda, Masahito
title_short Evaluation of effective astrophysical S factor for non-resonant reactions.
title_full Evaluation of effective astrophysical S factor for non-resonant reactions.
title_fullStr Evaluation of effective astrophysical S factor for non-resonant reactions.
title_full_unstemmed Evaluation of effective astrophysical S factor for non-resonant reactions.
title_sort Evaluation of effective astrophysical S factor for non-resonant reactions.
author Ueda, Masahito
author_facet Ueda, Masahito
Sargeant, Adam James
Pato, Mauricio Porto
Hussein, Mahir Saleh
author_role author
author2 Sargeant, Adam James
Pato, Mauricio Porto
Hussein, Mahir Saleh
author2_role author
author
author
dc.contributor.author.fl_str_mv Ueda, Masahito
Sargeant, Adam James
Pato, Mauricio Porto
Hussein, Mahir Saleh
description 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.
publishDate 2001
dc.date.issued.fl_str_mv 2001
dc.date.accessioned.fl_str_mv 2012-09-27T13:23:53Z
dc.date.available.fl_str_mv 2012-09-27T13:23:53Z
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
dc.type.driver.fl_str_mv info:eu-repo/semantics/conferenceObject
format conferenceObject
status_str publishedVersion
dc.identifier.citation.fl_str_mv 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.
dc.identifier.uri.fl_str_mv http://www.repositorio.ufop.br/handle/123456789/1450
identifier_str_mv 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.
url http://www.repositorio.ufop.br/handle/123456789/1450
dc.language.iso.fl_str_mv eng
language eng
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