Dark matter from a radiative inverse seesaw majoron model

dc.creatorBonilla, Cesar
dc.creatorCárcamo Hernández, A. E.
dc.creatorDíaz Sáez, Bastián
dc.creatorKovalenko, Sergey
dc.creatorMarchant González, Juan
dc.date.accessioned2023-11-22T11:33:27Z
dc.date.accessioned2024-05-02T15:06:01Z
dc.date.available2023-11-22T11:33:27Z
dc.date.available2024-05-02T15:06:01Z
dc.date.created2023-11-22T11:33:27Z
dc.date.issued2023-11-10
dc.identifierPhysics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, Volume 847, 10 December 2023, Article number 138282
dc.identifier03702693
dc.identifierhttps://repositorio.unab.cl/xmlui/handle/ria/54014
dc.identifier10.1016/j.physletb.2023.138282
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/9262398
dc.description.abstractWe 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)
dc.languageen
dc.publisherElsevier B.V.
dc.rightshttps://creativecommons.org/licenses/by/4.0/
dc.rightsCC BY 4.0 DEED Attribution 4.0 International
dc.titleDark matter from a radiative inverse seesaw majoron model
dc.typeArtículo


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