Matter-parity as a residual gauge symmetry: Probing a theory of cosmological dark matter

Detalhes bibliográficos
Autor(a) principal: Alves, Alexandre [UNIFESP]
Data de Publicação: 2017
Outros Autores: Arcadi, Giorgio, Dong, P. V., Duarte, Laura, Queiroz, Farinaldo S., Valle, Jose W. F.
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UNIFESP
Texto Completo: https://repositorio.unifesp.br/handle/11600/57368
http://dx.doi.org/10.1016/j.physletb.2017.07.056
Resumo: We discuss a non-supersymmetric scenario which addresses the origin of the matter-parity symmetry, P-M = (-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. (C) 2017 The Author(s). Published by Elsevier B.V.
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spelling Alves, Alexandre [UNIFESP]Arcadi, GiorgioDong, P. V.Duarte, LauraQueiroz, Farinaldo S.Valle, Jose W. F.2020-08-04T13:40:12Z2020-08-04T13:40:12Z2017Physics Letters B. Amsterdam, v. 772, p. 825-831, 2017.0370-2693https://repositorio.unifesp.br/handle/11600/57368http://dx.doi.org/10.1016/j.physletb.2017.07.056WOS000411369700116.pdf10.1016/j.physletb.2017.07.056WOS:000411369700116We discuss a non-supersymmetric scenario which addresses the origin of the matter-parity symmetry, P-M = (-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. (C) 2017 The Author(s). Published by Elsevier B.V.Brazilian agency CNPqBrazilian agency FAPESPSpanish grantsVietnam National Foundation for Science and Technology Development (NAFOSTED)CAPESUniv Fed Sao Paulo, Dept Fis, BR-09972270 Diadema, SP, BrazilMax Planck Inst Kernphys, Saupfercheckweg 1, D-69117 Heidelberg, GermanyVietnam Acad Sci & Technol, Inst Phys, 10 Dao Tan, Hanoi, VietnamUNESP, Dept Fis & Quim, Campus Guaratingueta, Guaratingueta, SP, BrazilUniv Valencia, CSIC, Edificio Inst Paterna, AHEP Grp,Inst Fis Corpuscular, C Catedrat Jose Beltran 2, E-46980 Paterna, Valencia, SpainUniv Fed Sao Paulo, Dept Fis, BR-09972270 Diadema, SP, BrazilCNPq: 307098/2014-1FAPESP: 2013/22079-8Web of Science825-831engElsevier Science BvPhysics Letters BMatter-parity as a residual gauge symmetry: Probing a theory of cosmological dark matterinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articleAmsterdam772info:eu-repo/semantics/openAccessreponame:Repositório Institucional da UNIFESPinstname:Universidade Federal de São Paulo (UNIFESP)instacron:UNIFESPORIGINALWOS000411369700116.pdfapplication/pdf742225${dspace.ui.url}/bitstream/11600/57368/1/WOS000411369700116.pdfe22c4d9fbb4a1dd6ff3f85ed2dd50894MD51open accessTEXTWOS000411369700116.pdf.txtWOS000411369700116.pdf.txtExtracted texttext/plain38872${dspace.ui.url}/bitstream/11600/57368/8/WOS000411369700116.pdf.txtb787de9431caf3676abe857aa035a6b2MD58open accessTHUMBNAILWOS000411369700116.pdf.jpgWOS000411369700116.pdf.jpgIM Thumbnailimage/jpeg7012${dspace.ui.url}/bitstream/11600/57368/10/WOS000411369700116.pdf.jpg1ac929d481cb14f6f0e649823d676877MD510open access11600/573682023-06-05 19:27:08.944open accessoai:repositorio.unifesp.br:11600/57368Repositório InstitucionalPUBhttp://www.repositorio.unifesp.br/oai/requestopendoar:34652023-06-05T22:27:08Repositório Institucional da UNIFESP - Universidade Federal de São Paulo (UNIFESP)false
dc.title.en.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 [UNIFESP]
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 [UNIFESP]
author_facet Alves, Alexandre [UNIFESP]
Arcadi, Giorgio
Dong, P. V.
Duarte, Laura
Queiroz, Farinaldo S.
Valle, Jose W. F.
author_role author
author2 Arcadi, Giorgio
Dong, P. V.
Duarte, Laura
Queiroz, Farinaldo S.
Valle, Jose W. F.
author2_role author
author
author
author
author
dc.contributor.author.fl_str_mv Alves, Alexandre [UNIFESP]
Arcadi, Giorgio
Dong, P. V.
Duarte, Laura
Queiroz, Farinaldo S.
Valle, Jose W. F.
description We discuss a non-supersymmetric scenario which addresses the origin of the matter-parity symmetry, P-M = (-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. (C) 2017 The Author(s). Published by Elsevier B.V.
publishDate 2017
dc.date.issued.fl_str_mv 2017
dc.date.accessioned.fl_str_mv 2020-08-04T13:40:12Z
dc.date.available.fl_str_mv 2020-08-04T13:40:12Z
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dc.identifier.citation.fl_str_mv Physics Letters B. Amsterdam, v. 772, p. 825-831, 2017.
dc.identifier.uri.fl_str_mv https://repositorio.unifesp.br/handle/11600/57368
http://dx.doi.org/10.1016/j.physletb.2017.07.056
dc.identifier.issn.none.fl_str_mv 0370-2693
dc.identifier.file.none.fl_str_mv WOS000411369700116.pdf
dc.identifier.doi.none.fl_str_mv 10.1016/j.physletb.2017.07.056
dc.identifier.wos.none.fl_str_mv WOS:000411369700116
identifier_str_mv Physics Letters B. Amsterdam, v. 772, p. 825-831, 2017.
0370-2693
WOS000411369700116.pdf
10.1016/j.physletb.2017.07.056
WOS:000411369700116
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