Closing the SU(3)L U(1)X symmetry at the electroweak scale

Detalhes bibliográficos
Autor(a) principal: Dias, Alex G.
Data de Publicação: 2006
Outros Autores: Montero, J. C. [UNESP], Pleitez, V. [UNESP]
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.1103/PhysRevD.73.113004
http://hdl.handle.net/11449/224768
Resumo: We show that some models with SU(3)C SU(3)L U(1)X gauge symmetry can be realized at the electroweak scale and that this is a consequence of an approximate global SU(2)L+R symmetry. This symmetry implies a condition among the vacuum expectation value of one of the neutral Higgs scalars, the U(1)X's coupling constant, gX, the sine of the weak mixing angle sin θW, and the mass of the W boson, MW. In the limit in which this symmetry is valid it avoids the tree level mixing of the Z boson of the standard model with the extra Z′ boson. We have verified that the oblique T parameter is within the allowed range indicating that the radiative corrections that induce such a mixing at the 1-loop level are small. We also show that a SU(3)L+R custodial symmetry implies that in some of the models we have to include sterile (singlets of the 3-3-1 symmetry) right-handed neutrinos with Majorana masses, since the seesaw mechanism is mandatory to obtain light active neutrinos. Moreover, the approximate SU(2)L+R SU(3)L+R symmetry implies that the extra nonstandard particles of these 3-3-1 models can be considerably lighter than it had been thought before so that new physics can be really just around the corner. © 2006 The American Physical Society.
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spelling Closing the SU(3)L U(1)X symmetry at the electroweak scaleWe show that some models with SU(3)C SU(3)L U(1)X gauge symmetry can be realized at the electroweak scale and that this is a consequence of an approximate global SU(2)L+R symmetry. This symmetry implies a condition among the vacuum expectation value of one of the neutral Higgs scalars, the U(1)X's coupling constant, gX, the sine of the weak mixing angle sin θW, and the mass of the W boson, MW. In the limit in which this symmetry is valid it avoids the tree level mixing of the Z boson of the standard model with the extra Z′ boson. We have verified that the oblique T parameter is within the allowed range indicating that the radiative corrections that induce such a mixing at the 1-loop level are small. We also show that a SU(3)L+R custodial symmetry implies that in some of the models we have to include sterile (singlets of the 3-3-1 symmetry) right-handed neutrinos with Majorana masses, since the seesaw mechanism is mandatory to obtain light active neutrinos. Moreover, the approximate SU(2)L+R SU(3)L+R symmetry implies that the extra nonstandard particles of these 3-3-1 models can be considerably lighter than it had been thought before so that new physics can be really just around the corner. © 2006 The American Physical Society.Instituto de Física Universidade de São Paulo, C.P. 66.318, 05315-970 São Paulo, SPInstituto de Física Teórica Universidade Estadual Paulista, Rua Pamplona 145, 01405-000, São Paulo, SPInstituto de Física Teórica Universidade Estadual Paulista, Rua Pamplona 145, 01405-000, São Paulo, SPUniversidade de São Paulo (USP)Universidade Estadual Paulista (UNESP)Dias, Alex G.Montero, J. C. [UNESP]Pleitez, V. [UNESP]2022-04-28T20:08:14Z2022-04-28T20:08:14Z2006-06-23info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articlehttp://dx.doi.org/10.1103/PhysRevD.73.113004Physical Review D - Particles, Fields, Gravitation and Cosmology, v. 73, n. 11, 2006.1550-79981550-2368http://hdl.handle.net/11449/22476810.1103/PhysRevD.73.1130042-s2.0-33745163985Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengPhysical Review D - Particles, Fields, Gravitation and Cosmologyinfo:eu-repo/semantics/openAccess2022-04-28T20:08:14Zoai:repositorio.unesp.br:11449/224768Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T13:56:56.678458Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Closing the SU(3)L U(1)X symmetry at the electroweak scale
title Closing the SU(3)L U(1)X symmetry at the electroweak scale
spellingShingle Closing the SU(3)L U(1)X symmetry at the electroweak scale
Dias, Alex G.
title_short Closing the SU(3)L U(1)X symmetry at the electroweak scale
title_full Closing the SU(3)L U(1)X symmetry at the electroweak scale
title_fullStr Closing the SU(3)L U(1)X symmetry at the electroweak scale
title_full_unstemmed Closing the SU(3)L U(1)X symmetry at the electroweak scale
title_sort Closing the SU(3)L U(1)X symmetry at the electroweak scale
author Dias, Alex G.
author_facet Dias, Alex G.
Montero, J. C. [UNESP]
Pleitez, V. [UNESP]
author_role author
author2 Montero, J. C. [UNESP]
Pleitez, V. [UNESP]
author2_role author
author
dc.contributor.none.fl_str_mv Universidade de São Paulo (USP)
Universidade Estadual Paulista (UNESP)
dc.contributor.author.fl_str_mv Dias, Alex G.
Montero, J. C. [UNESP]
Pleitez, V. [UNESP]
description We show that some models with SU(3)C SU(3)L U(1)X gauge symmetry can be realized at the electroweak scale and that this is a consequence of an approximate global SU(2)L+R symmetry. This symmetry implies a condition among the vacuum expectation value of one of the neutral Higgs scalars, the U(1)X's coupling constant, gX, the sine of the weak mixing angle sin θW, and the mass of the W boson, MW. In the limit in which this symmetry is valid it avoids the tree level mixing of the Z boson of the standard model with the extra Z′ boson. We have verified that the oblique T parameter is within the allowed range indicating that the radiative corrections that induce such a mixing at the 1-loop level are small. We also show that a SU(3)L+R custodial symmetry implies that in some of the models we have to include sterile (singlets of the 3-3-1 symmetry) right-handed neutrinos with Majorana masses, since the seesaw mechanism is mandatory to obtain light active neutrinos. Moreover, the approximate SU(2)L+R SU(3)L+R symmetry implies that the extra nonstandard particles of these 3-3-1 models can be considerably lighter than it had been thought before so that new physics can be really just around the corner. © 2006 The American Physical Society.
publishDate 2006
dc.date.none.fl_str_mv 2006-06-23
2022-04-28T20:08:14Z
2022-04-28T20:08:14Z
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.73.113004
Physical Review D - Particles, Fields, Gravitation and Cosmology, v. 73, n. 11, 2006.
1550-7998
1550-2368
http://hdl.handle.net/11449/224768
10.1103/PhysRevD.73.113004
2-s2.0-33745163985
url http://dx.doi.org/10.1103/PhysRevD.73.113004
http://hdl.handle.net/11449/224768
identifier_str_mv Physical Review D - Particles, Fields, Gravitation and Cosmology, v. 73, n. 11, 2006.
1550-7998
1550-2368
10.1103/PhysRevD.73.113004
2-s2.0-33745163985
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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