Publicação: Secluded and putative flipped dark matter and Stueckelberg extensions of the standard model
dc.contributor.author | Fortes, E. C. F. S. | |
dc.contributor.author | Pleitez, V. [UNESP] | |
dc.contributor.author | Stecker, F. W. | |
dc.contributor.institution | Univ Fed Pampa | |
dc.contributor.institution | Universidade Estadual Paulista (Unesp) | |
dc.contributor.institution | NASA | |
dc.date.accessioned | 2018-11-26T17:48:14Z | |
dc.date.available | 2018-11-26T17:48:14Z | |
dc.date.issued | 2018-02-01 | |
dc.description.abstract | We 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.affiliation | Univ Fed Pampa, Rua Luiz Joaquin de Sa Brito S-N, BR-97650000 Itaqui, RS, Brazil | |
dc.description.affiliation | Univ Estadual Paulista, Inst Fis Teor, Rua Dr Bento Teobaldo Ferraz 271, BR-01110070 Sao Paulo, SP, Brazil | |
dc.description.affiliation | NASA, Goddard Space Flight Ctr, Astrophys Sci Div, Greenbelt, MD 20771 USA | |
dc.description.affiliationUnesp | Univ Estadual Paulista, Inst Fis Teor, Rua Dr Bento Teobaldo Ferraz 271, BR-01110070 Sao Paulo, SP, Brazil | |
dc.description.sponsorship | Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq) | |
dc.description.sponsorship | Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP) | |
dc.description.sponsorshipId | FAPESP: 2014/19164-6 | |
dc.format.extent | 13 | |
dc.identifier | http://dx.doi.org/10.1088/1475-7516/2018/02/026 | |
dc.identifier.citation | Journal Of Cosmology And Astroparticle Physics. Bristol: Iop Publishing Ltd, n. 2, 13 p., 2018. | |
dc.identifier.doi | 10.1088/1475-7516/2018/02/026 | |
dc.identifier.file | WOS000425350700001.pdf | |
dc.identifier.issn | 1475-7516 | |
dc.identifier.uri | http://hdl.handle.net/11449/163872 | |
dc.identifier.wos | WOS:000425350700001 | |
dc.language.iso | eng | |
dc.publisher | Iop Publishing Ltd | |
dc.relation.ispartof | Journal Of Cosmology And Astroparticle Physics | |
dc.relation.ispartofsjr | 1,089 | |
dc.rights.accessRights | Acesso aberto | |
dc.source | Web of Science | |
dc.subject | dark matter theory | |
dc.subject | gamma ray theory | |
dc.title | Secluded and putative flipped dark matter and Stueckelberg extensions of the standard model | en |
dc.type | Artigo | |
dcterms.license | http://iopscience.iop.org/page/copyright | |
dcterms.rightsHolder | Iop Publishing Ltd | |
dspace.entity.type | Publication | |
unesp.campus | Universidade Estadual Paulista (UNESP), Instituto de Física Teórica (IFT), São Paulo | pt |
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