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Please use this identifier to cite or link to this item: http://acervodigital.unesp.br/handle/11449/65942
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dc.contributor.authorMontero, J. C.-
dc.contributor.authorPires, C. A D S-
dc.contributor.authorPleitez, V.-
dc.date.accessioned2014-05-27T11:19:49Z-
dc.date.accessioned2016-10-25T18:16:00Z-
dc.date.available2014-05-27T11:19:49Z-
dc.date.available2016-10-25T18:16:00Z-
dc.date.issued1999-12-01-
dc.identifierhttp://dx.doi.org/10.1103/PhysRevD.60.115003-
dc.identifier.citationPhysical Review D - Particles, Fields, Gravitation and Cosmology, v. 60, n. 11, p. 1-6, 1999.-
dc.identifier.issn0556-2821-
dc.identifier.urihttp://hdl.handle.net/11449/65942-
dc.identifier.urihttp://acervodigital.unesp.br/handle/11449/65942-
dc.description.abstractIn a 3-3-1 model in which the lepton masses arise from a scalar sextet it is possible to break spontaneously a global symmetry which implies in a pseudoscalar Majoron-like Goldstone boson. This Majoron does not mix with any other scalar fields and for this reason it does not couple, at the tree level, to either the charged leptons or to the quarks. Moreover, its interaction with neutrinos is diagonal. We also argue that there is a set of parameters in which the model can be consistent with the invisible Z0 width and that heavy neutrinos can decay sufficiently rapid by Majoron emission, having a lifetime shorter than the age of the universe. ©1999 The American Physical Society.en
dc.format.extent1-6-
dc.language.isoeng-
dc.sourceScopus-
dc.titleSpontaneous breaking of a global symmetry in a 3-3-1 modelen
dc.typeoutro-
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)-
dc.description.affiliationInst. de Fis. Teórica Universidade Estadual Paulista, Rua Pamplona 145, 01405-900 São Paulo, S.P.-
dc.description.affiliationUnespInst. de Fis. Teórica Universidade Estadual Paulista, Rua Pamplona 145, 01405-900 São Paulo, S.P.-
dc.identifier.doi10.1103/PhysRevD.60.115003-
dc.identifier.wosWOS:000084138100075-
dc.rights.accessRightsAcesso restrito-
dc.identifier.file2-s2.0-18044388597.pdf-
dc.relation.ispartofPhysical Review D: Particles, Fields, Gravitation and Cosmology-
dc.identifier.scopus2-s2.0-18044388597-
dc.identifier.orcid0000-0001-5279-8438pt
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