Invisible axion and neutrino masses
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.73.017701 http://hdl.handle.net/11449/224715 |
Resumo: | We show that in any invisible axion model due to the effects of effective nonrenormalizable interactions related to an energy scale near the Peccei-Quinn, grand unification or even the Planck scale, active neutrinos necessarily acquire masses in the sub-eV range. Moreover, if sterile neutrinos are also included and if appropriate cyclic ZN symmetries are imposed, it is possible that some of these neutrinos are heavy while others are light. © 2006 The American Physical Society. |
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Repositório Institucional da UNESP |
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Invisible axion and neutrino massesWe show that in any invisible axion model due to the effects of effective nonrenormalizable interactions related to an energy scale near the Peccei-Quinn, grand unification or even the Planck scale, active neutrinos necessarily acquire masses in the sub-eV range. Moreover, if sterile neutrinos are also included and if appropriate cyclic ZN symmetries are imposed, it is possible that some of these neutrinos are heavy while others are light. © 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, São Paulo, SPInstituto de Física, Teórica, Universidade Estadual Paulista, Rua Pamplona 145, São Paulo, SPUniversidade de São Paulo (USP)Universidade Estadual Paulista (UNESP)Dias, Alex G.Pleitez, V. [UNESP]2022-04-28T20:07:10Z2022-04-28T20:07:10Z2006-01-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articlehttp://dx.doi.org/10.1103/PhysRevD.73.017701Physical Review D - Particles, Fields, Gravitation and Cosmology, v. 73, n. 1, 2006.1550-23681550-7998http://hdl.handle.net/11449/22471510.1103/PhysRevD.73.0177012-s2.0-32644468560Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengPhysical Review D - Particles, Fields, Gravitation and Cosmologyinfo:eu-repo/semantics/openAccess2022-04-28T20:07:10Zoai:repositorio.unesp.br:11449/224715Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T22:56:19.250227Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false |
dc.title.none.fl_str_mv |
Invisible axion and neutrino masses |
title |
Invisible axion and neutrino masses |
spellingShingle |
Invisible axion and neutrino masses Dias, Alex G. |
title_short |
Invisible axion and neutrino masses |
title_full |
Invisible axion and neutrino masses |
title_fullStr |
Invisible axion and neutrino masses |
title_full_unstemmed |
Invisible axion and neutrino masses |
title_sort |
Invisible axion and neutrino masses |
author |
Dias, Alex G. |
author_facet |
Dias, Alex G. Pleitez, V. [UNESP] |
author_role |
author |
author2 |
Pleitez, V. [UNESP] |
author2_role |
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. Pleitez, V. [UNESP] |
description |
We show that in any invisible axion model due to the effects of effective nonrenormalizable interactions related to an energy scale near the Peccei-Quinn, grand unification or even the Planck scale, active neutrinos necessarily acquire masses in the sub-eV range. Moreover, if sterile neutrinos are also included and if appropriate cyclic ZN symmetries are imposed, it is possible that some of these neutrinos are heavy while others are light. © 2006 The American Physical Society. |
publishDate |
2006 |
dc.date.none.fl_str_mv |
2006-01-01 2022-04-28T20:07:10Z 2022-04-28T20:07:10Z |
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.73.017701 Physical Review D - Particles, Fields, Gravitation and Cosmology, v. 73, n. 1, 2006. 1550-2368 1550-7998 http://hdl.handle.net/11449/224715 10.1103/PhysRevD.73.017701 2-s2.0-32644468560 |
url |
http://dx.doi.org/10.1103/PhysRevD.73.017701 http://hdl.handle.net/11449/224715 |
identifier_str_mv |
Physical Review D - Particles, Fields, Gravitation and Cosmology, v. 73, n. 1, 2006. 1550-2368 1550-7998 10.1103/PhysRevD.73.017701 2-s2.0-32644468560 |
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 |
|
_version_ |
1808129475981869056 |