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Please use this identifier to cite or link to this item: http://acervodigital.unesp.br/handle/11449/64922
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dc.contributor.authorPisano, F.-
dc.contributor.authorTomazelli, J. L.-
dc.date.accessioned2014-05-27T11:18:09Z-
dc.date.accessioned2016-10-25T18:14:07Z-
dc.date.available2014-05-27T11:18:09Z-
dc.date.available2016-10-25T18:14:07Z-
dc.date.issued1996-12-01-
dc.identifierhttp://dx.doi.org/10.1142/S0217732396000667-
dc.identifier.citationModern Physics Letters A, v. 11, n. 8, p. 647-651, 1996.-
dc.identifier.issn0217-7323-
dc.identifier.urihttp://hdl.handle.net/11449/64922-
dc.identifier.urihttp://acervodigital.unesp.br/handle/11449/64922-
dc.description.abstractA class of boson-fermion stars, whose spin-0 and spin-1/2 constituents interact through a U(1) current-current term in the Lagrangian density, is analyzed. It is shown that it describes the low-energy behavior of a system of weakly interacting massive particles (WIMPs) from the leptonic sector of the minimal supersymmetric standard model. In this case the effective coupling constant A is related to the Fermi constant GF.en
dc.format.extent647-651-
dc.language.isoeng-
dc.sourceScopus-
dc.titleStars of WIMPsen
dc.typeoutro-
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)-
dc.description.affiliationInst. de Fís. Teórica Universidade Estadual Paulista, Rua Pamplona, 145 01405-000 São Paulo, SP-
dc.description.affiliationUnespInst. de Fís. Teórica Universidade Estadual Paulista, Rua Pamplona, 145 01405-000 São Paulo, SP-
dc.identifier.doi10.1142/S0217732396000667-
dc.identifier.wosWOS:A1996UG11900005-
dc.rights.accessRightsAcesso restrito-
dc.relation.ispartofModern Physics Letters A-
dc.identifier.scopus2-s2.0-0542380941-
Appears in Collections:Artigos, TCCs, Teses e Dissertações da Unesp

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