Gravitino dark matter and neutrino masses with bilinear R-parity violation

ABSTRACT: The origin of neutrino masses and mixing and the nature of dark matter are two of the most elusive open problems of modern particle physics and cosmology, which clearly indicate the need for new physics beyond the standard model. It has been suggested that these two apparently unrelated is...

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Autores:
Taoso, Marco
Valle, José W. F.
Zapata Noreña, Óscar Alberto
Restrepo Quintero, Diego Alejandro
Tipo de recurso:
Article of investigation
Fecha de publicación:
2012
Institución:
Universidad de Antioquia
Repositorio:
Repositorio UdeA
Idioma:
eng
OAI Identifier:
oai:bibliotecadigital.udea.edu.co:10495/8364
Acceso en línea:
http://hdl.handle.net/10495/8364
Palabra clave:
Cosmología
Cosmology
Neutrinos
Neutrines
Física nuclear
Nuclear physics
Mezclas de neutrinos
Materia oscura (Astronomía)
Física de partículas
http://aims.fao.org/aos/agrovoc/c_49984
http://vocabularies.unesco.org/thesaurus/concept3235
Rights
openAccess
License
https://creativecommons.org/licenses/by-nc-nd/4.0/
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dc.title.spa.fl_str_mv Gravitino dark matter and neutrino masses with bilinear R-parity violation
title Gravitino dark matter and neutrino masses with bilinear R-parity violation
spellingShingle Gravitino dark matter and neutrino masses with bilinear R-parity violation
Cosmología
Cosmology
Neutrinos
Neutrines
Física nuclear
Nuclear physics
Mezclas de neutrinos
Materia oscura (Astronomía)
Física de partículas
http://aims.fao.org/aos/agrovoc/c_49984
http://vocabularies.unesco.org/thesaurus/concept3235
title_short Gravitino dark matter and neutrino masses with bilinear R-parity violation
title_full Gravitino dark matter and neutrino masses with bilinear R-parity violation
title_fullStr Gravitino dark matter and neutrino masses with bilinear R-parity violation
title_full_unstemmed Gravitino dark matter and neutrino masses with bilinear R-parity violation
title_sort Gravitino dark matter and neutrino masses with bilinear R-parity violation
dc.creator.fl_str_mv Taoso, Marco
Valle, José W. F.
Zapata Noreña, Óscar Alberto
Restrepo Quintero, Diego Alejandro
dc.contributor.author.none.fl_str_mv Taoso, Marco
Valle, José W. F.
Zapata Noreña, Óscar Alberto
Restrepo Quintero, Diego Alejandro
dc.contributor.researchgroup.spa.fl_str_mv Grupo de Fenomenologia de Interacciones Fundamentales
dc.subject.unesco.none.fl_str_mv Cosmología
Cosmology
topic Cosmología
Cosmology
Neutrinos
Neutrines
Física nuclear
Nuclear physics
Mezclas de neutrinos
Materia oscura (Astronomía)
Física de partículas
http://aims.fao.org/aos/agrovoc/c_49984
http://vocabularies.unesco.org/thesaurus/concept3235
dc.subject.lemb.none.fl_str_mv Neutrinos
Neutrines
dc.subject.agrovoc.none.fl_str_mv Física nuclear
Nuclear physics
dc.subject.proposal.spa.fl_str_mv Mezclas de neutrinos
Materia oscura (Astronomía)
Física de partículas
dc.subject.agrovocuri.none.fl_str_mv http://aims.fao.org/aos/agrovoc/c_49984
dc.subject.unescouri.none.fl_str_mv http://vocabularies.unesco.org/thesaurus/concept3235
description ABSTRACT: The origin of neutrino masses and mixing and the nature of dark matter are two of the most elusive open problems of modern particle physics and cosmology, which clearly indicate the need for new physics beyond the standard model. It has been suggested that these two apparently unrelated issues may be closely interlinked. Here we propose an alternative way to relate dark matter with neutrino properties within a scenario where supersymmetry (SUSY) is the origin of neutrino mass, thanks to the spontaneous violation of R parity. For definiteness and simplicity we adopt an effective description in terms of explicit bilinear R-parity violating superpotential terms (BRpV)
publishDate 2012
dc.date.issued.none.fl_str_mv 2012
dc.date.accessioned.none.fl_str_mv 2017-09-27T15:54:33Z
dc.date.available.none.fl_str_mv 2017-09-27T15:54:33Z
dc.type.spa.fl_str_mv Artículo de investigación
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dc.identifier.citation.spa.fl_str_mv Restrepo Quintero, D. A., Taoso, M., Valle, J. W. F., & Zapata Noreña, O. A. (2012). Gravitino dark matter and neutrino masses with bilinear R-parity violation. Physical Review D. 85(023523), 1-7.
dc.identifier.issn.none.fl_str_mv 2470-0010
dc.identifier.uri.none.fl_str_mv http://hdl.handle.net/10495/8364
dc.identifier.doi.none.fl_str_mv 10.1103/PhysRevD.85.023523
dc.identifier.eissn.none.fl_str_mv 2470-0029
identifier_str_mv Restrepo Quintero, D. A., Taoso, M., Valle, J. W. F., & Zapata Noreña, O. A. (2012). Gravitino dark matter and neutrino masses with bilinear R-parity violation. Physical Review D. 85(023523), 1-7.
2470-0010
10.1103/PhysRevD.85.023523
2470-0029
url http://hdl.handle.net/10495/8364
dc.language.iso.spa.fl_str_mv eng
language eng
dc.relation.ispartofjournalabbrev.spa.fl_str_mv Phys. Rev. D
dc.relation.citationendpage.spa.fl_str_mv 7
dc.relation.citationissue.spa.fl_str_mv 23523
dc.relation.citationstartpage.spa.fl_str_mv 1
dc.relation.citationvolume.spa.fl_str_mv 85
dc.relation.ispartofjournal.spa.fl_str_mv Physical Review D
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dc.publisher.spa.fl_str_mv The American Physical Society
dc.publisher.place.spa.fl_str_mv Estados Unidos
institution Universidad de Antioquia
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spelling Taoso, MarcoValle, José W. F.Zapata Noreña, Óscar AlbertoRestrepo Quintero, Diego Alejandrovirtual::50-1Grupo de Fenomenologia de Interacciones Fundamentales2017-09-27T15:54:33Z2017-09-27T15:54:33Z2012Restrepo Quintero, D. A., Taoso, M., Valle, J. W. F., & Zapata Noreña, O. A. (2012). Gravitino dark matter and neutrino masses with bilinear R-parity violation. Physical Review D. 85(023523), 1-7.2470-0010http://hdl.handle.net/10495/836410.1103/PhysRevD.85.0235232470-0029ABSTRACT: The origin of neutrino masses and mixing and the nature of dark matter are two of the most elusive open problems of modern particle physics and cosmology, which clearly indicate the need for new physics beyond the standard model. It has been suggested that these two apparently unrelated issues may be closely interlinked. Here we propose an alternative way to relate dark matter with neutrino properties within a scenario where supersymmetry (SUSY) is the origin of neutrino mass, thanks to the spontaneous violation of R parity. 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