The dark matter puzzle in a class of models with gauge symmetry SU(3)C ⊗ SU(3)L ⊗ U(1)N
| dc.creator | Carlos Enrique Alvarez Salazar | |
| dc.creator | Orlando Luis Goulart Peres | |
| dc.creator | Bruce Lehmann Sánchez Vega | |
| dc.date.accessioned | 2023-07-17T18:15:23Z | |
| dc.date.accessioned | 2025-09-09T00:46:50Z | |
| dc.date.available | 2023-07-17T18:15:23Z | |
| dc.date.issued | 2019 | |
| dc.description.sponsorship | CNPq - Conselho Nacional de Desenvolvimento Científico e Tecnológico | |
| dc.description.sponsorship | FAPESP - Fundação de Amparo à Pesquisa do Estado de São Paulo | |
| dc.identifier.doi | https://doi.org/10.1002/asna.201913577 | |
| dc.identifier.issn | 1521-3994 | |
| dc.identifier.uri | https://hdl.handle.net/1843/56424 | |
| dc.language | eng | |
| dc.publisher | Universidade Federal de Minas Gerais | |
| dc.relation.ispartof | Astronomische Nachrichten | |
| dc.rights | Acesso Restrito | |
| dc.subject | Matéria escura | |
| dc.subject | Partículas elementares | |
| dc.subject.other | Dark matter | |
| dc.subject.other | Elementary particles | |
| dc.title | The dark matter puzzle in a class of models with gauge symmetry SU(3)C ⊗ SU(3)L ⊗ U(1)N | |
| dc.type | Artigo de periódico | |
| local.citation.epage | 138 | |
| local.citation.issue | 1-3 | |
| local.citation.spage | 135 | |
| local.citation.volume | 340 | |
| local.description.resumo | We analyze the dark matter (DM) puzzle in a class of models with gauge symmetry SU(3)C ⊗ SU(3)L ⊗ U(1)N, taking into account the constraints coming from Planck observations of the DM relic density, direct detection searches with Xenon1T, and indirect detection using Fermi-LAT data. The model has two possible candidates, a fermion and a scalar, which require, to evade the constraints set by Xenon1T and Fermi-LAT, and have relic densities in the range measured by the Planck collaboration, a minimum vacuum expectation value to break the SU(3)L symmetry of 10 and 15 TeV, respectively. In this case, these particles have masses of order 1 TeV, for the fermion, and between 500 and 600 GeV, for the scalar. | |
| local.identifier.orcid | https://orcid.org/0000-0003-3107-446X | |
| local.identifier.orcid | https://orcid.org/0000-0003-2104-8460 | |
| local.identifier.orcid | https://orcid.org/0000-0002-6735-5813 | |
| local.publisher.country | Brasil | |
| local.publisher.department | ICX - DEPARTAMENTO DE FÍSICA | |
| local.publisher.initials | UFMG | |
| local.url.externa | https://onlinelibrary.wiley.com/doi/10.1002/asna.201913577 |
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