Natural Peccei-Quinn symmetry in the 3-3-1 model with a minimal scalar sector
Autor(a) principal: | |
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Data de Publicação: | 2011 |
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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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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) |
repository.mail.fl_str_mv |
|
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1808129515455512576 |