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Please use this identifier to cite or link to this item: http://acervodigital.unesp.br/handle/11449/35540
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dc.contributor.authorNatale, A. A.-
dc.contributor.authorDasilva, PSR-
dc.date.accessioned2014-05-20T15:25:04Z-
dc.date.accessioned2016-10-25T17:59:25Z-
dc.date.available2014-05-20T15:25:04Z-
dc.date.available2016-10-25T17:59:25Z-
dc.date.issued1995-08-20-
dc.identifierhttp://dx.doi.org/10.1142/S0217732395001964-
dc.identifier.citationModern Physics Letters A. Singapore: World Scientific Publ Co Pte Ltd, v. 10, n. 25, p. 1829-1836, 1995.-
dc.identifier.issn0217-7323-
dc.identifier.urihttp://hdl.handle.net/11449/35540-
dc.identifier.urihttp://acervodigital.unesp.br/handle/11449/35540-
dc.description.abstractWe compute the one-loop oblique corrections in a typical model with neutrino masses due to the seesaw mechanism. We verify that a Dirac neutrino mass up to 178 GeV is still allowed by the experimental data.en
dc.format.extent1829-1836-
dc.language.isoeng-
dc.publisherWorld Scientific Publ Co Pte Ltd-
dc.sourceWeb of Science-
dc.titleLIMIT ON A HEAVY DIRAC NEUTRINO THROUGH OBLIQUE RADIATIVE-CORRECTIONSen
dc.typeoutro-
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)-
dc.description.affiliationUNIV ESTADUAL PAULISTA,INST FIS TEOR,RUA PAMPLONA 145,BR-01405 SAO PAULO,BRAZIL-
dc.description.affiliationUnespUNIV ESTADUAL PAULISTA,INST FIS TEOR,RUA PAMPLONA 145,BR-01405 SAO PAULO,BRAZIL-
dc.identifier.doi10.1142/S0217732395001964-
dc.identifier.wosWOS:A1995RT43000003-
dc.rights.accessRightsAcesso restrito-
dc.relation.ispartofModern Physics Letters A-
Appears in Collections:Artigos, TCCs, Teses e Dissertações da Unesp

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