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Natural Peccei-Quinn symmetry in the 3-3-1 model with a minimal scalar sector

dc.contributor.authorMontero, J. C. [UNESP]
dc.contributor.authorSánchez-Vega, B. L. [UNESP]
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)
dc.date.accessioned2022-04-29T01:01:57Z
dc.date.available2022-04-29T01:01:57Z
dc.date.issued2011-09-22
dc.description.abstractIn the framework of a 3-3-1 model with a minimal scalar sector we make a detailed study concerning the implementation of the Peccei-Quinn symmetry in order to solve the strong CP problem. For the original version of the model, with only two scalar triplets, we show that the entire Lagrangian is invariant under a Peccei-Quinn-like symmetry but no axion is produced since a U(1) subgroup remains unbroken. Although in this case the strong CP problem can still be solved, the solution is largely disfavored since three quark states are left massless to all orders in perturbation theory. The addition of a third scalar triplet removes the massless quark states but the resulting axion is visible. In order to become realistic the model must be extended to account for massive quarks and an invisible axion. We show that the addition of a scalar singlet together with a ZN discrete gauge symmetry can successfully accomplish these tasks and protect the axion field against quantum gravitational effects. To make sure that the protecting discrete gauge symmetry is anomaly-free we use a discrete version of the Green-Schwarz mechanism. © 2011 American Physical Society.en
dc.description.affiliationInstituto de Física Teórica Universidade Estadual Paulista, R. Dr. Bento Teobaldo Ferraz 271, Barra Funda, São Paulo-SP, 01140-070
dc.description.affiliationUnespInstituto de Física Teórica Universidade Estadual Paulista, R. Dr. Bento Teobaldo Ferraz 271, Barra Funda, São Paulo-SP, 01140-070
dc.identifierhttp://dx.doi.org/10.1103/PhysRevD.84.055019
dc.identifier.citationPhysical Review D - Particles, Fields, Gravitation and Cosmology, v. 84, n. 5, 2011.
dc.identifier.dimensionspub.1008671078
dc.identifier.doi10.1103/PhysRevD.84.055019
dc.identifier.issn1550-7998
dc.identifier.issn1550-2368
dc.identifier.issn2470-0010
dc.identifier.issn1089-4918
dc.identifier.orcid0000-0002-5457-9359
dc.identifier.orcid0000-0002-6735-5813
dc.identifier.scopus2-s2.0-80053531539
dc.identifier.urihttp://hdl.handle.net/11449/226545
dc.language.isoeng
dc.publisherAmerican Physical Society (APS)
dc.relation.ispartofPhysical Review D - Particles, Fields, Gravitation and Cosmology
dc.rights.accessRightsAcesso abertopt
dc.rights.sourceRightsoa_all
dc.rights.sourceRightsgreen
dc.sourceScopus
dc.sourceDimensions
dc.titleNatural Peccei-Quinn symmetry in the 3-3-1 model with a minimal scalar sectoren
dc.typeArtigopt
dspace.entity.typePublication
relation.isOrgUnitOfPublication41d94a5b-139b-457c-90a7-77b71f4e94df
relation.isOrgUnitOfPublication.latestForDiscovery41d94a5b-139b-457c-90a7-77b71f4e94df
unesp.campusUniversidade Estadual Paulista (UNESP), Instituto de Física Teórica (IFT), São Paulopt

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