Please use this identifier to cite or link to this item: http://repositorio.unicamp.br/jspui/handle/REPOSIP/341259
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dc.contributor.CRUESPUNIVERSIDADE ESTADUAL DE CAMPINASpt_BR
dc.contributor.authorunicampRomero Castellanos, Ana Rubielapt_BR
dc.contributor.authorunicampAlvarez Salazar, Carlos Enriquept_BR
dc.typeArtigopt_BR
dc.titleConstraints on axionic dark matter in the 3-3-1 modelpt_BR
dc.contributor.authorCastellanos, A. R.pt_BR
dc.contributor.authorAlvarez-Salazar, C. E.pt_BR
dc.contributor.authorSanchez-Vega, B. L.pt_BR
dc.subjectPartículas (Física nuclear)pt_BR
dc.subjectMatéria escura (Astronomia)pt_BR
dc.subject.otherlanguageParticles (Nuclear physics)pt_BR
dc.subject.otherlanguageDark matter (Astronomy)pt_BR
dc.description.abstractDark matter in the form of axions can be included in models with SU(3)(C) circle times SU(3)(L) circle times U(1)(X) symmetry with right-handed neutrinos, where the strong charge-parity (CP) problem can be solved. Different versions of the model have the appealing characteristic of giving the observed dark matter abundance, measured by the Planck collaboration, for suitable values of the parameters. We studied the constraints on the parameter space of the model obtained when the axion mass is calculated taking into account both quantum chromodynamics (QCD) effects and gravitationally induced operators, making a comparison of three different models.pt_BR
dc.relation.ispartofAstronomische nachrichtenpt_BR
dc.relation.ispartofabbreviationAstron. nachr.pt_BR
dc.publisher.cityWeinheimpt_BR
dc.publisher.countryAlemanhapt_BR
dc.publisherWiley-VCH Verlagpt_BR
dc.date.issued2019pt_BR
dc.date.monthofcirculationJan./Mar.pt_BR
dc.language.isoengpt_BR
dc.description.volume340pt_BR
dc.description.issuenumber1/3pt_BR
dc.description.issuespecialSIpt_BR
dc.description.firstpage131pt_BR
dc.description.lastpage134pt_BR
dc.rightsfechadopt_BR
dc.sourceWOSpt_BR
dc.identifier.issn0004-6337pt_BR
dc.identifier.eissn1521-3994pt_BR
dc.identifier.doi10.1002/asna.201913576pt_BR
dc.identifier.urlhttps://onlinelibrary.wiley.com/doi/full/10.1002/asna.201913576pt_BR
dc.description.sponsorshipCONSELHO NACIONAL DE DESENVOLVIMENTO CIENTÍFICO E TECNOLÓGICO - CNPQpt_BR
dc.description.sponsorshipCOORDENAÇÃO DE APERFEIÇOAMENTO DE PESSOAL DE NÍVEL SUPERIOR - CAPESpt_BR
dc.description.sponsorshipFUNDAÇÃO DE AMPARO À PESQUISA DO ESTADO DE SÃO PAULO - FAPESPpt_BR
dc.description.sponsorship1FAPESP - FUNDAÇÃO DE AMPARO À PESQUISA DO ESTADO DE SÃO PAULOpt_BR
dc.description.sponsorship1CNPQ - CONSELHO NACIONAL DE DESENVOLVIMENTO CIENTÍFICO E TECNOLÓGICOpt_BR
dc.description.sponsorship1CAPES - COORDENAÇÃO DE APERFEIÇOAMENTO DE PESSOAL E NÍVEL SUPERIORpt_BR
dc.description.sponsordocumentnumber2014/19164-6pt_BR
dc.description.sponsordocumentnumber159237/2015-7pt_BR
dc.description.sponsordocumentnumberSem informaçãopt_BR
dc.date.available2020-05-13T19:34:58Z-
dc.date.accessioned2020-05-13T19:34:58Z-
dc.description.provenanceMade available in DSpace on 2020-05-13T19:34:58Z (GMT). No. of bitstreams: 1 000468591100026.pdf: 439325 bytes, checksum: 8b72f4d40740dc8e78bc534c983ef9ba (MD5) Previous issue date: 2019en
dc.identifier.urihttp://repositorio.unicamp.br/jspui/handle/REPOSIP/341259-
dc.description.conferencenome8. International Workshop on Astronomy and Relativistic Astrophysics (IWARA)pt_BR
dc.contributor.departmentDepartamento de Raios Cósmicos e Cronologiapt_BR
dc.contributor.departmentDepartamento de Raios Cósmicos e Cronologiapt_BR
dc.contributor.unidadeInstituto de Física "Gleb Wataghin"pt_BR
dc.identifier.source000468591100026pt_BR
dc.creator.orcid0000-0002-6115-229Xpt_BR
dc.creator.orcid0000-0003-3107-446Xpt_BR
dc.type.formArtigo de eventopt_BR
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