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Please use this identifier to cite or link to this item: http://acervodigital.unesp.br/handle/11449/33529
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dc.contributor.authorFoot, R.-
dc.contributor.authorHernandez, O. F.-
dc.contributor.authorPisano, F.-
dc.contributor.authorPLEITEZ, V-
dc.date.accessioned2014-05-20T15:22:35Z-
dc.date.accessioned2016-10-25T17:56:17Z-
dc.date.available2014-05-20T15:22:35Z-
dc.date.available2016-10-25T17:56:17Z-
dc.date.issued1993-05-01-
dc.identifierhttp://dx.doi.org/10.1103/PhysRevD.47.4158-
dc.identifier.citationPhysical Review D. College Pk: American Physical Soc, v. 47, n. 9, p. 4158-4161, 1993.-
dc.identifier.issn0556-2821-
dc.identifier.urihttp://hdl.handle.net/11449/33529-
dc.identifier.urihttp://acervodigital.unesp.br/handle/11449/33529-
dc.description.abstractThe SU(3)cxSU(3)LxU(1)N model of Pisano and Pleitez extends the standard model in a particularly nice way, so that, for example, the anomalies cancel only when the number of generations is divisible by 3. The original version of the model has some problems accounting for the lepton masses. We resolve this problem by modifying the details of the symmetry-breaking sector in the model.en
dc.format.extent4158-4161-
dc.language.isoeng-
dc.publisherAmerican Physical Soc-
dc.sourceWeb of Science-
dc.titleLEPTON MASSES IN AN SU(3)L-CIRCLE-TIMES-U(1)N GAUGE-MODELen
dc.typeoutro-
dc.contributor.institutionMCGILL UNIV-
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)-
dc.description.affiliationMCGILL UNIV,DEPT PHYS,MONTREAL H3A 2T8,QUEBEC,CANADA-
dc.description.affiliationUNIV ESTADUAL PAULISTA,INST FIS TEOR,BR-01405-900 SAO PAULO,BRAZIL-
dc.description.affiliationUnespUNIV ESTADUAL PAULISTA,INST FIS TEOR,BR-01405-900 SAO PAULO,BRAZIL-
dc.identifier.doi10.1103/PhysRevD.47.4158-
dc.identifier.wosWOS:A1993LA92800059-
dc.rights.accessRightsAcesso restrito-
dc.identifier.fileWOSA1993LA92800059.pdf-
dc.relation.ispartofPhysical Review D-
dc.identifier.orcid0000-0001-5279-8438pt
Appears in Collections:Artigos, TCCs, Teses e Dissertações da Unesp

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