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

Detalhes bibliográficos
Autor(a) principal: Montero, J. C. [UNESP]
Data de Publicação: 2011
Outros Autores: Sánchez-Vega, B. L. [UNESP]
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.1103/PhysRevD.84.055019
http://hdl.handle.net/11449/226545
Resumo: In 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.
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spelling Natural Peccei-Quinn symmetry in the 3-3-1 model with a minimal scalar sectorIn 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.Instituto de Física Teórica Universidade Estadual Paulista, R. Dr. Bento Teobaldo Ferraz 271, Barra Funda, São Paulo-SP, 01140-070Instituto de Física Teórica Universidade Estadual Paulista, R. Dr. Bento Teobaldo Ferraz 271, Barra Funda, São Paulo-SP, 01140-070Universidade Estadual Paulista (UNESP)Montero, J. C. [UNESP]Sánchez-Vega, B. L. [UNESP]2022-04-29T01:01:57Z2022-04-29T01:01:57Z2011-09-22info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articlehttp://dx.doi.org/10.1103/PhysRevD.84.055019Physical Review D - Particles, Fields, Gravitation and Cosmology, v. 84, n. 5, 2011.1550-79981550-2368http://hdl.handle.net/11449/22654510.1103/PhysRevD.84.0550192-s2.0-80053531539Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengPhysical Review D - Particles, Fields, Gravitation and Cosmologyinfo:eu-repo/semantics/openAccess2022-04-29T01:01:57Zoai:repositorio.unesp.br:11449/226545Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T23:23:38.655934Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Natural Peccei-Quinn symmetry in the 3-3-1 model with a minimal scalar sector
title Natural Peccei-Quinn symmetry in the 3-3-1 model with a minimal scalar sector
spellingShingle Natural Peccei-Quinn symmetry in the 3-3-1 model with a minimal scalar sector
Montero, J. C. [UNESP]
title_short Natural Peccei-Quinn symmetry in the 3-3-1 model with a minimal scalar sector
title_full Natural Peccei-Quinn symmetry in the 3-3-1 model with a minimal scalar sector
title_fullStr Natural Peccei-Quinn symmetry in the 3-3-1 model with a minimal scalar sector
title_full_unstemmed Natural Peccei-Quinn symmetry in the 3-3-1 model with a minimal scalar sector
title_sort Natural Peccei-Quinn symmetry in the 3-3-1 model with a minimal scalar sector
author Montero, J. C. [UNESP]
author_facet Montero, J. C. [UNESP]
Sánchez-Vega, B. L. [UNESP]
author_role author
author2 Sánchez-Vega, B. L. [UNESP]
author2_role author
dc.contributor.none.fl_str_mv Universidade Estadual Paulista (UNESP)
dc.contributor.author.fl_str_mv Montero, J. C. [UNESP]
Sánchez-Vega, B. L. [UNESP]
description In 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.
publishDate 2011
dc.date.none.fl_str_mv 2011-09-22
2022-04-29T01:01:57Z
2022-04-29T01:01:57Z
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
dc.type.driver.fl_str_mv info:eu-repo/semantics/article
format article
status_str publishedVersion
dc.identifier.uri.fl_str_mv http://dx.doi.org/10.1103/PhysRevD.84.055019
Physical Review D - Particles, Fields, Gravitation and Cosmology, v. 84, n. 5, 2011.
1550-7998
1550-2368
http://hdl.handle.net/11449/226545
10.1103/PhysRevD.84.055019
2-s2.0-80053531539
url http://dx.doi.org/10.1103/PhysRevD.84.055019
http://hdl.handle.net/11449/226545
identifier_str_mv Physical Review D - Particles, Fields, Gravitation and Cosmology, v. 84, n. 5, 2011.
1550-7998
1550-2368
10.1103/PhysRevD.84.055019
2-s2.0-80053531539
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Physical Review D - Particles, Fields, Gravitation and Cosmology
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.source.none.fl_str_mv Scopus
reponame:Repositório Institucional da UNESP
instname:Universidade Estadual Paulista (UNESP)
instacron:UNESP
instname_str Universidade Estadual Paulista (UNESP)
instacron_str UNESP
institution UNESP
reponame_str Repositório Institucional da UNESP
collection Repositório Institucional da UNESP
repository.name.fl_str_mv Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)
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