Naturally light invisible axion in models with large local discrete symmetries

Detalhes bibliográficos
Autor(a) principal: Dias, Alex G.
Data de Publicação: 2003
Outros Autores: Pleitez, V. [UNESP], Tonasse, M. D.
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.1103/PhysRevD.67.095008
http://hdl.handle.net/11449/224320
Resumo: We show that by introducing appropriate local [Formula Presented] symmetries in electroweak models it is possible to implement an automatic Peccei-Quinn symmetry, at the same time keeping the axion protected against gravitational effects. Although we consider here only an extension of the standard model and a particular 3-3-1 model, the strategy can be used in any kind of electroweak model. An interesting feature of this 3-3-1 model is that if we add (i) right-handed neutrinos, (ii) the conservation of the total lepton number, and (iii) a [Formula Presented] symmetry, the [Formula Presented] and the chiral Peccei-Quinn [Formula Presented] symmetries are both accidental symmetries in the sense that they are not imposed on the Lagrangian but are just a consequence of the particle content of the model, its gauge invariance, renormalizability, and Lorentz invariance. In addition, this model has no domain wall problem. © 2003 The American Physical Society.
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spelling Naturally light invisible axion in models with large local discrete symmetriesWe show that by introducing appropriate local [Formula Presented] symmetries in electroweak models it is possible to implement an automatic Peccei-Quinn symmetry, at the same time keeping the axion protected against gravitational effects. Although we consider here only an extension of the standard model and a particular 3-3-1 model, the strategy can be used in any kind of electroweak model. An interesting feature of this 3-3-1 model is that if we add (i) right-handed neutrinos, (ii) the conservation of the total lepton number, and (iii) a [Formula Presented] symmetry, the [Formula Presented] and the chiral Peccei-Quinn [Formula Presented] symmetries are both accidental symmetries in the sense that they are not imposed on the Lagrangian but are just a consequence of the particle content of the model, its gauge invariance, renormalizability, and Lorentz invariance. In addition, this model has no domain wall problem. © 2003 The American Physical Society.Instituto de Física Universidade de São Paulo, São Paulo, 05315-970Instituto de Física Teórica Universidade Estadual Paulista, 01405-900Instituto Tecnológico de Aeronáutica Centro Técnico Aeroespacial, 12228-901Instituto de Física Teórica Universidade Estadual Paulista, 01405-900Universidade de São Paulo (USP)Universidade Estadual Paulista (UNESP)Centro Técnico AeroespacialDias, Alex G.Pleitez, V. [UNESP]Tonasse, M. D.2022-04-28T19:55:56Z2022-04-28T19:55:56Z2003-01-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articlehttp://dx.doi.org/10.1103/PhysRevD.67.095008Physical Review D - Particles, Fields, Gravitation and Cosmology, v. 67, n. 9, 2003.1550-23681550-7998http://hdl.handle.net/11449/22432010.1103/PhysRevD.67.0950082-s2.0-0038575108Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengPhysical Review D - Particles, Fields, Gravitation and Cosmologyinfo:eu-repo/semantics/openAccess2022-04-28T19:55:56Zoai:repositorio.unesp.br:11449/224320Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462022-04-28T19:55:56Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Naturally light invisible axion in models with large local discrete symmetries
title Naturally light invisible axion in models with large local discrete symmetries
spellingShingle Naturally light invisible axion in models with large local discrete symmetries
Dias, Alex G.
title_short Naturally light invisible axion in models with large local discrete symmetries
title_full Naturally light invisible axion in models with large local discrete symmetries
title_fullStr Naturally light invisible axion in models with large local discrete symmetries
title_full_unstemmed Naturally light invisible axion in models with large local discrete symmetries
title_sort Naturally light invisible axion in models with large local discrete symmetries
author Dias, Alex G.
author_facet Dias, Alex G.
Pleitez, V. [UNESP]
Tonasse, M. D.
author_role author
author2 Pleitez, V. [UNESP]
Tonasse, M. D.
author2_role author
author
dc.contributor.none.fl_str_mv Universidade de São Paulo (USP)
Universidade Estadual Paulista (UNESP)
Centro Técnico Aeroespacial
dc.contributor.author.fl_str_mv Dias, Alex G.
Pleitez, V. [UNESP]
Tonasse, M. D.
description We show that by introducing appropriate local [Formula Presented] symmetries in electroweak models it is possible to implement an automatic Peccei-Quinn symmetry, at the same time keeping the axion protected against gravitational effects. Although we consider here only an extension of the standard model and a particular 3-3-1 model, the strategy can be used in any kind of electroweak model. An interesting feature of this 3-3-1 model is that if we add (i) right-handed neutrinos, (ii) the conservation of the total lepton number, and (iii) a [Formula Presented] symmetry, the [Formula Presented] and the chiral Peccei-Quinn [Formula Presented] symmetries are both accidental symmetries in the sense that they are not imposed on the Lagrangian but are just a consequence of the particle content of the model, its gauge invariance, renormalizability, and Lorentz invariance. In addition, this model has no domain wall problem. © 2003 The American Physical Society.
publishDate 2003
dc.date.none.fl_str_mv 2003-01-01
2022-04-28T19:55:56Z
2022-04-28T19:55:56Z
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.67.095008
Physical Review D - Particles, Fields, Gravitation and Cosmology, v. 67, n. 9, 2003.
1550-2368
1550-7998
http://hdl.handle.net/11449/224320
10.1103/PhysRevD.67.095008
2-s2.0-0038575108
url http://dx.doi.org/10.1103/PhysRevD.67.095008
http://hdl.handle.net/11449/224320
identifier_str_mv Physical Review D - Particles, Fields, Gravitation and Cosmology, v. 67, n. 9, 2003.
1550-2368
1550-7998
10.1103/PhysRevD.67.095008
2-s2.0-0038575108
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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