Closing the SU(3)L U(1)X symmetry at the electroweak scale
Autor(a) principal: | |
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Data de Publicação: | 2006 |
Outros Autores: | , |
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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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) |
repository.mail.fl_str_mv |
|
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1808128293555142656 |