Matter-parity as a residual gauge symmetry: Probing a theory of cosmological dark matter
Autor(a) principal: | |
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Data de Publicação: | 2017 |
Outros Autores: | , , , , |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UNESP |
Texto Completo: | http://dx.doi.org/10.1016/j.physletb.2017.07.056 http://hdl.handle.net/11449/175000 |
Resumo: | We discuss a non-supersymmetric scenario which addresses the origin of the matter-parity symmetry, PM=(−1)3(B−L)+2s, leading to a viable Dirac fermion dark matter candidate. Implications to electroweak precision, muon anomalous magnetic moment, flavor changing interactions, lepton flavor violation, dark matter and collider physics are discussed in detail. We show that this non-supersymmetric model is capable of generating the matter-parity symmetry in agreement with existing data with gripping implications to particle physics and cosmology. |
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Repositório Institucional da UNESP |
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spelling |
Matter-parity as a residual gauge symmetry: Probing a theory of cosmological dark matterWe discuss a non-supersymmetric scenario which addresses the origin of the matter-parity symmetry, PM=(−1)3(B−L)+2s, leading to a viable Dirac fermion dark matter candidate. Implications to electroweak precision, muon anomalous magnetic moment, flavor changing interactions, lepton flavor violation, dark matter and collider physics are discussed in detail. We show that this non-supersymmetric model is capable of generating the matter-parity symmetry in agreement with existing data with gripping implications to particle physics and cosmology.Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)National Foundation for Science and Technology DevelopmentFundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)Ministerio de Economía y CompetitividadDepartamento de Física Universidade Federal de São PauloMax-Planck-Institut für Kernphysik, Saupfercheckweg 1Institute of Physics Vietnam Academy of Science and Technology, 10 Dao Tan, Ba DinhUNESP Departamento de Física e Quḿica, Campus de GuaratinguetáAHEP Group Instituto de Física Corpuscular C.S.I.C./Universitat de Valencia Edificio de Institutos de Paterna, C/Catedratico José Beltran, 2UNESP Departamento de Física e Quḿica, Campus de GuaratinguetáNational Foundation for Science and Technology Development: 103.01-2016.77FAPESP: 2013/22079-8CNPq: 307098/2014-1Ministerio de Economía y Competitividad: CSD2009-00064Ministerio de Economía y Competitividad: FPA2014-58183-PMinisterio de Economía y Competitividad: SEV-2014-0398Universidade Federal de São Paulo (UNIFESP)Max-Planck-Institut für KernphysikVietnam Academy of Science and TechnologyUniversidade Estadual Paulista (Unesp)Edificio de Institutos de PaternaAlves, AlexandreArcadi, GiorgioDong, P. V.Duarte, Laura [UNESP]Queiroz, Farinaldo S.Valle, José W.F.2018-12-11T17:13:47Z2018-12-11T17:13:47Z2017-09-10info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/article825-831application/pdfhttp://dx.doi.org/10.1016/j.physletb.2017.07.056Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, v. 772, p. 825-831.0370-2693http://hdl.handle.net/11449/17500010.1016/j.physletb.2017.07.0562-s2.0-850267808392-s2.0-85026780839.pdfScopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengPhysics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics2,336info:eu-repo/semantics/openAccess2023-12-23T06:19:29Zoai:repositorio.unesp.br:11449/175000Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462023-12-23T06:19:29Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false |
dc.title.none.fl_str_mv |
Matter-parity as a residual gauge symmetry: Probing a theory of cosmological dark matter |
title |
Matter-parity as a residual gauge symmetry: Probing a theory of cosmological dark matter |
spellingShingle |
Matter-parity as a residual gauge symmetry: Probing a theory of cosmological dark matter Alves, Alexandre |
title_short |
Matter-parity as a residual gauge symmetry: Probing a theory of cosmological dark matter |
title_full |
Matter-parity as a residual gauge symmetry: Probing a theory of cosmological dark matter |
title_fullStr |
Matter-parity as a residual gauge symmetry: Probing a theory of cosmological dark matter |
title_full_unstemmed |
Matter-parity as a residual gauge symmetry: Probing a theory of cosmological dark matter |
title_sort |
Matter-parity as a residual gauge symmetry: Probing a theory of cosmological dark matter |
author |
Alves, Alexandre |
author_facet |
Alves, Alexandre Arcadi, Giorgio Dong, P. V. Duarte, Laura [UNESP] Queiroz, Farinaldo S. Valle, José W.F. |
author_role |
author |
author2 |
Arcadi, Giorgio Dong, P. V. Duarte, Laura [UNESP] Queiroz, Farinaldo S. Valle, José W.F. |
author2_role |
author author author author author |
dc.contributor.none.fl_str_mv |
Universidade Federal de São Paulo (UNIFESP) Max-Planck-Institut für Kernphysik Vietnam Academy of Science and Technology Universidade Estadual Paulista (Unesp) Edificio de Institutos de Paterna |
dc.contributor.author.fl_str_mv |
Alves, Alexandre Arcadi, Giorgio Dong, P. V. Duarte, Laura [UNESP] Queiroz, Farinaldo S. Valle, José W.F. |
description |
We discuss a non-supersymmetric scenario which addresses the origin of the matter-parity symmetry, PM=(−1)3(B−L)+2s, leading to a viable Dirac fermion dark matter candidate. Implications to electroweak precision, muon anomalous magnetic moment, flavor changing interactions, lepton flavor violation, dark matter and collider physics are discussed in detail. We show that this non-supersymmetric model is capable of generating the matter-parity symmetry in agreement with existing data with gripping implications to particle physics and cosmology. |
publishDate |
2017 |
dc.date.none.fl_str_mv |
2017-09-10 2018-12-11T17:13:47Z 2018-12-11T17:13:47Z |
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/10.1016/j.physletb.2017.07.056 Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, v. 772, p. 825-831. 0370-2693 http://hdl.handle.net/11449/175000 10.1016/j.physletb.2017.07.056 2-s2.0-85026780839 2-s2.0-85026780839.pdf |
url |
http://dx.doi.org/10.1016/j.physletb.2017.07.056 http://hdl.handle.net/11449/175000 |
identifier_str_mv |
Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, v. 772, p. 825-831. 0370-2693 10.1016/j.physletb.2017.07.056 2-s2.0-85026780839 2-s2.0-85026780839.pdf |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics 2,336 |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
dc.format.none.fl_str_mv |
825-831 application/pdf |
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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1792962154403463168 |