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Please use this identifier to cite or link to this item: http://acervodigital.unesp.br/handle/11449/23141
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dc.contributor.authorDias, A. G.-
dc.contributor.authorPleitez, V-
dc.date.accessioned2014-05-20T14:05:56Z-
dc.date.available2014-05-20T14:05:56Z-
dc.date.issued2004-04-01-
dc.identifierhttp://dx.doi.org/10.1103/PhysRevD.69.077702-
dc.identifier.citationPhysical Review D. College Pk: American Physical Soc, v. 69, n. 7, 4 p., 2004.-
dc.identifier.issn0556-2821-
dc.identifier.urihttp://hdl.handle.net/11449/23141-
dc.description.abstractBy introducing local Z(N) symmetries with N=11,13 in two 3-3-1 models, it is possible to implement an automatic Peccei-Quinn symmetry, keeping the axion protected against gravitational effects at the same time. Both models have a Z(2) domain wall problem and the neutrinos are strictly Dirac particles.en
dc.format.extent4-
dc.language.isoeng-
dc.publisherAmerican Physical Soc-
dc.sourceWeb of Science-
dc.titleStabilizing the invisible axion in 3-3-1 modelsen
dc.typeoutro-
dc.contributor.institutionUniversidade de São Paulo (USP)-
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)-
dc.description.affiliationUniv São Paulo, Inst Fis, BR-05315970 São Paulo, Brazil-
dc.description.affiliationUniv Estadual Paulista, Inst Fis Teor, BR-01405900 São Paulo, Brazil-
dc.description.affiliationUnespUniv Estadual Paulista, Inst Fis Teor, BR-01405900 São Paulo, Brazil-
dc.identifier.doi10.1103/PhysRevD.69.077702-
dc.identifier.wosWOS:000221253900093-
dc.rights.accessRightsAcesso restrito-
dc.identifier.fileWOS000221253900093.pdf-
dc.relation.ispartofPhysical Review D-
dc.identifier.orcid0000-0001-5279-8438pt
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