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

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dc.contributor.authorAlves, Alexandre
dc.contributor.authorArcadi, Giorgio
dc.contributor.authorDong, P. V.
dc.contributor.authorDuarte, Laura [UNESP]
dc.contributor.authorQueiroz, Farinaldo S.
dc.contributor.authorValle, José W.F.
dc.contributor.institutionUniversidade Federal de São Paulo (UNIFESP)
dc.contributor.institutionMax-Planck-Institut für Kernphysik
dc.contributor.institutionVietnam Academy of Science and Technology
dc.contributor.institutionUniversidade Estadual Paulista (Unesp)
dc.contributor.institutionEdificio de Institutos de Paterna
dc.date.accessioned2018-12-11T17:13:47Z
dc.date.available2018-12-11T17:13:47Z
dc.date.issued2017-09-10
dc.description.abstractWe 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.en
dc.description.affiliationDepartamento de Física Universidade Federal de São Paulo
dc.description.affiliationMax-Planck-Institut für Kernphysik, Saupfercheckweg 1
dc.description.affiliationInstitute of Physics Vietnam Academy of Science and Technology, 10 Dao Tan, Ba Dinh
dc.description.affiliationUNESP Departamento de Física e Quḿica, Campus de Guaratinguetá
dc.description.affiliationAHEP Group Instituto de Física Corpuscular C.S.I.C./Universitat de Valencia Edificio de Institutos de Paterna, C/Catedratico José Beltran, 2
dc.description.affiliationUnespUNESP Departamento de Física e Quḿica, Campus de Guaratinguetá
dc.description.sponsorshipCoordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)
dc.description.sponsorshipNational Foundation for Science and Technology Development
dc.description.sponsorshipFundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)
dc.description.sponsorshipConselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)
dc.description.sponsorshipMinisterio de Economía y Competitividad
dc.description.sponsorshipIdNational Foundation for Science and Technology Development: 103.01-2016.77
dc.description.sponsorshipIdFAPESP: 2013/22079-8
dc.description.sponsorshipIdCNPq: 307098/2014-1
dc.description.sponsorshipIdMinisterio de Economía y Competitividad: CSD2009-00064
dc.description.sponsorshipIdMinisterio de Economía y Competitividad: FPA2014-58183-P
dc.description.sponsorshipIdMinisterio de Economía y Competitividad: SEV-2014-0398
dc.format.extent825-831
dc.identifierhttp://dx.doi.org/10.1016/j.physletb.2017.07.056
dc.identifier.citationPhysics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, v. 772, p. 825-831.
dc.identifier.doi10.1016/j.physletb.2017.07.056
dc.identifier.file2-s2.0-85026780839.pdf
dc.identifier.issn0370-2693
dc.identifier.scopus2-s2.0-85026780839
dc.identifier.urihttp://hdl.handle.net/11449/175000
dc.language.isoeng
dc.relation.ispartofPhysics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
dc.relation.ispartofsjr2,336
dc.rights.accessRightsAcesso aberto
dc.sourceScopus
dc.titleMatter-parity as a residual gauge symmetry: Probing a theory of cosmological dark matteren
dc.typeArtigo
unesp.author.orcid0000-0002-7141-5532[5]
unesp.departmentFísica e Química - FEGpt

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Guaratinguetá - FEG - Faculdade de Engenharia e Ciências