Publicação:
Secluded and putative flipped dark matter and Stueckelberg extensions of the standard model

dc.contributor.authorFortes, E. C. F. S.
dc.contributor.authorPleitez, V. [UNESP]
dc.contributor.authorStecker, F. W.
dc.contributor.institutionUniv Fed Pampa
dc.contributor.institutionUniversidade Estadual Paulista (Unesp)
dc.contributor.institutionNASA
dc.date.accessioned2018-11-26T17:48:14Z
dc.date.available2018-11-26T17:48:14Z
dc.date.issued2018-02-01
dc.description.abstractWe consider here three dark matter models with the gauge symmetry of the standard model plus an additional local U(1)(D) factor. One model is truly secluded and the other two models begin flipped, but end up secluded. All of these models include one dark fermion and one vector boson that gains mass via the Stueckelberg mechanism. We show that the would be flipped models provide an example dark matter composed of almost least interacting particles (ALIPs). Such particles are therefore compatible with the constraints obtained from both laboratory measurements and astrophysical observations.en
dc.description.affiliationUniv Fed Pampa, Rua Luiz Joaquin de Sa Brito S-N, BR-97650000 Itaqui, RS, Brazil
dc.description.affiliationUniv Estadual Paulista, Inst Fis Teor, Rua Dr Bento Teobaldo Ferraz 271, BR-01110070 Sao Paulo, SP, Brazil
dc.description.affiliationNASA, Goddard Space Flight Ctr, Astrophys Sci Div, Greenbelt, MD 20771 USA
dc.description.affiliationUnespUniv Estadual Paulista, Inst Fis Teor, Rua Dr Bento Teobaldo Ferraz 271, BR-01110070 Sao Paulo, SP, Brazil
dc.description.sponsorshipConselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)
dc.description.sponsorshipFundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)
dc.description.sponsorshipIdFAPESP: 2014/19164-6
dc.format.extent13
dc.identifierhttp://dx.doi.org/10.1088/1475-7516/2018/02/026
dc.identifier.citationJournal Of Cosmology And Astroparticle Physics. Bristol: Iop Publishing Ltd, n. 2, 13 p., 2018.
dc.identifier.doi10.1088/1475-7516/2018/02/026
dc.identifier.fileWOS000425350700001.pdf
dc.identifier.issn1475-7516
dc.identifier.urihttp://hdl.handle.net/11449/163872
dc.identifier.wosWOS:000425350700001
dc.language.isoeng
dc.publisherIop Publishing Ltd
dc.relation.ispartofJournal Of Cosmology And Astroparticle Physics
dc.relation.ispartofsjr1,089
dc.rights.accessRightsAcesso aberto
dc.sourceWeb of Science
dc.subjectdark matter theory
dc.subjectgamma ray theory
dc.titleSecluded and putative flipped dark matter and Stueckelberg extensions of the standard modelen
dc.typeArtigo
dcterms.licensehttp://iopscience.iop.org/page/copyright
dcterms.rightsHolderIop Publishing Ltd
dspace.entity.typePublication
unesp.campusUniversidade Estadual Paulista (UNESP), Instituto de Física Teórica (IFT), São Paulopt

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