Dark matter from a radiative inverse seesaw majoron model
dc.contributor.author | Bonilla, Cesar | |
dc.contributor.author | Cárcamo Hernández, A. E. | |
dc.contributor.author | Díaz Sáez, Bastián | |
dc.contributor.author | Kovalenko, Sergey | |
dc.contributor.author | Marchant González, Juan | |
dc.date.accessioned | 2023-11-22T11:33:27Z | |
dc.date.available | 2023-11-22T11:33:27Z | |
dc.date.issued | 2023-11-10 | |
dc.description | INDEXACIÓN: SCOPUS. | es |
dc.description.abstract | We propose a Majoron-like extension of the Standard Model with an extra global U(1)X-symmetry where neutrino masses are generated through an inverse seesaw mechanism at the 1-loop level. In contrast to the tree-level inverse seesaw, our framework contains dark matter (DM) candidates stabilized by a residual Z2-symmetry surviving spontaneous breaking of the U(1)X-group. We explore the case in which the DM is a Majorana fermion. Furthermore, we provide parameter space regions allowed by current experimental constraints coming from the dark matter relic abundance, (in)direct detection, and charged lepton flavor violation. © 2023 The Author(s) | es |
dc.identifier.citation | Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, Volume 847, 10 December 2023, Article number 138282 | es |
dc.identifier.doi | 10.1016/j.physletb.2023.138282 | |
dc.identifier.issn | 03702693 | |
dc.identifier.uri | https://repositorio.unab.cl/xmlui/handle/ria/54014 | |
dc.language.iso | en | es |
dc.publisher | Elsevier B.V. | es |
dc.rights.license | CC BY 4.0 DEED Attribution 4.0 International | |
dc.rights.uri | https://creativecommons.org/licenses/by/4.0/ | |
dc.title | Dark matter from a radiative inverse seesaw majoron model | es |
dc.type | Artículo | es |
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