Supersymmetric 3-3-1 model with right-handed neutrinos

Detalhes bibliográficos
Autor(a) principal: Montero, J. C. [UNESP]
Data de Publicação: 2004
Outros Autores: Pleitez, V. [UNESP], Rodriguez, M. C.
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.1103/PhysRevD.70.075004
http://hdl.handle.net/11449/224555
Resumo: We consider the supersymmetric extension of the 3-3-1 model with right-handed neutrinos. We study the mass spectra in the scalar and pseudoscalar sectors, and for a given set of the input parameters, we find that the lightest scalar in the model has a mass of 130 GeV and the lightest pseudoscalar has mass of 5 GeV. However, this pseudoscalar decouples from the [Formula Presented] at high energy scales since it is almost a singlet under [Formula Presented]. © 2004 The American Physical Society.
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spelling Supersymmetric 3-3-1 model with right-handed neutrinosWe consider the supersymmetric extension of the 3-3-1 model with right-handed neutrinos. We study the mass spectra in the scalar and pseudoscalar sectors, and for a given set of the input parameters, we find that the lightest scalar in the model has a mass of 130 GeV and the lightest pseudoscalar has mass of 5 GeV. However, this pseudoscalar decouples from the [Formula Presented] at high energy scales since it is almost a singlet under [Formula Presented]. © 2004 The American Physical Society.Instituto de Física Teórica Universidade Estadual Paulista, Rua Pamplona, 14501405-900Fundação Universidade Federal do Rio Grande/FURG Departamento de Física, Avenida Itália km 8, 96201-900Instituto de Física Teórica Universidade Estadual Paulista, Rua Pamplona, 14501405-900Universidade Estadual Paulista (UNESP)Fundação Universidade Federal do Rio Grande/FURGMontero, J. C. [UNESP]Pleitez, V. [UNESP]Rodriguez, M. C.2022-04-28T20:00:45Z2022-04-28T20:00:45Z2004-01-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articlehttp://dx.doi.org/10.1103/PhysRevD.70.075004Physical Review D - Particles, Fields, Gravitation and Cosmology, v. 70, n. 7, 2004.1550-23681550-7998http://hdl.handle.net/11449/22455510.1103/PhysRevD.70.0750042-s2.0-19744381746Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengPhysical Review D - Particles, Fields, Gravitation and Cosmologyinfo:eu-repo/semantics/openAccess2022-04-28T20:00:45Zoai:repositorio.unesp.br:11449/224555Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462022-04-28T20:00:45Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Supersymmetric 3-3-1 model with right-handed neutrinos
title Supersymmetric 3-3-1 model with right-handed neutrinos
spellingShingle Supersymmetric 3-3-1 model with right-handed neutrinos
Montero, J. C. [UNESP]
title_short Supersymmetric 3-3-1 model with right-handed neutrinos
title_full Supersymmetric 3-3-1 model with right-handed neutrinos
title_fullStr Supersymmetric 3-3-1 model with right-handed neutrinos
title_full_unstemmed Supersymmetric 3-3-1 model with right-handed neutrinos
title_sort Supersymmetric 3-3-1 model with right-handed neutrinos
author Montero, J. C. [UNESP]
author_facet Montero, J. C. [UNESP]
Pleitez, V. [UNESP]
Rodriguez, M. C.
author_role author
author2 Pleitez, V. [UNESP]
Rodriguez, M. C.
author2_role author
author
dc.contributor.none.fl_str_mv Universidade Estadual Paulista (UNESP)
Fundação Universidade Federal do Rio Grande/FURG
dc.contributor.author.fl_str_mv Montero, J. C. [UNESP]
Pleitez, V. [UNESP]
Rodriguez, M. C.
description We consider the supersymmetric extension of the 3-3-1 model with right-handed neutrinos. We study the mass spectra in the scalar and pseudoscalar sectors, and for a given set of the input parameters, we find that the lightest scalar in the model has a mass of 130 GeV and the lightest pseudoscalar has mass of 5 GeV. However, this pseudoscalar decouples from the [Formula Presented] at high energy scales since it is almost a singlet under [Formula Presented]. © 2004 The American Physical Society.
publishDate 2004
dc.date.none.fl_str_mv 2004-01-01
2022-04-28T20:00:45Z
2022-04-28T20:00:45Z
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.70.075004
Physical Review D - Particles, Fields, Gravitation and Cosmology, v. 70, n. 7, 2004.
1550-2368
1550-7998
http://hdl.handle.net/11449/224555
10.1103/PhysRevD.70.075004
2-s2.0-19744381746
url http://dx.doi.org/10.1103/PhysRevD.70.075004
http://hdl.handle.net/11449/224555
identifier_str_mv Physical Review D - Particles, Fields, Gravitation and Cosmology, v. 70, n. 7, 2004.
1550-2368
1550-7998
10.1103/PhysRevD.70.075004
2-s2.0-19744381746
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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