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Please use this identifier to cite or link to this item: http://hdl.handle.net/1843/56056
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dc.creatorCristian David Ruiz Carvajalpt_BR
dc.creatorBruce Lehmann Sánchez Vegapt_BR
dc.creatorÓscar Alberto Zapata Noreñapt_BR
dc.date.accessioned2023-07-11T12:22:12Z-
dc.date.available2023-07-11T12:22:12Z-
dc.date.issued2017-
dc.citation.volume96pt_BR
dc.citation.issue11pt_BR
dc.citation.spage115035-1pt_BR
dc.citation.epage15035-13pt_BR
dc.identifier.doihttps://doi.org/10.1103/PhysRevD.96.115035pt_BR
dc.identifier.issn2470-0029pt_BR
dc.identifier.urihttp://hdl.handle.net/1843/56056-
dc.description.resumoWe present a framework linking axionlike particles (ALPs) to neutrino masses through the minimal inverse seesaw (ISS) mechanism in order to explain the dark matter (DM) puzzle. Specifically, we explore three minimal ISS cases where mass scales are generated through gravity-induced operators involving a scalar field hosting ALPs. In all of these cases, we find gravity-stable models that provide the observed DM relic density and, simultaneously, are consistent with the phenomenology of neutrinos and ALPs. Remarkably, in one of the ISS cases, the DM can be made of ALPs and sterile neutrinos. Furthermore, other considered ISS cases have ALPs with parameters that are within the reach of proposed ALP experiments.pt_BR
dc.description.sponsorshipCAPES - Coordenação de Aperfeiçoamento de Pessoal de Nível Superiorpt_BR
dc.languageengpt_BR
dc.publisherUniversidade Federal de Minas Geraispt_BR
dc.publisher.countryBrasilpt_BR
dc.publisher.departmentICX - DEPARTAMENTO DE FÍSICApt_BR
dc.publisher.initialsUFMGpt_BR
dc.relation.ispartofPhysical Review D-
dc.rightsAcesso Restritopt_BR
dc.subjectAxion like particlespt_BR
dc.subjectNeutrinospt_BR
dc.subject.otherMatéria Escurapt_BR
dc.subject.otherNeutrinospt_BR
dc.titleLinking axionlike dark matter to neutrino massespt_BR
dc.typeArtigo de Periódicopt_BR
dc.url.externahttps://journals.aps.org/prd/abstract/10.1103/PhysRevD.96.115035pt_BR
dc.identifier.orcidhttps://orcid.org/0000-0002-5799-2464pt_BR
dc.identifier.orcidhttps://orcid.org/0000-0002-6735-5813pt_BR
dc.identifier.orcidhttps://orcid.org/0000-0001-5533-4014pt_BR
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