Scotogenic neutrino masses with gauged matter parity and gauge coupling unification

dc.creatorCárcamo Hernández, A.
dc.creatorHati, C.
dc.creatorKovalenko, S.
dc.creatorValle, J.
dc.creatorVaquera-Araujo, C.
dc.date.accessioned2022-06-22T14:25:58Z
dc.date.accessioned2024-05-02T15:05:03Z
dc.date.available2022-06-22T14:25:58Z
dc.date.available2024-05-02T15:05:03Z
dc.date.created2022-06-22T14:25:58Z
dc.date.issued2022-03
dc.identifierJournal of High Energy Physics, Volume 2022, Issue 3, March 2022, Article number 34
dc.identifier1029-8479
dc.identifierhttps://repositorio.unab.cl/xmlui/handle/ria/22931
dc.identifier10.1007/JHEP03(2022)034
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/9262128
dc.description.abstractBuilding up on previous work we propose a Dark Matter (DM) model with gauged matter parity and dynamical gauge coupling unification, driven by the same physics responsible for scotogenic neutrino mass generation. Our construction is based on the extended gauge group SU(3)c ⊗ SU(3)L ⊗ U(1)X ⊗ U(1)N, whose spontaneous breaking leaves a residual conserved matter parity, MP, stabilizing the DM particle candidates of the model. The key role is played by Majorana SU(3)L-octet leptons, allowing the successful gauge coupling unification and a one-loop scotogenic neutrino mass generation. Theoretical consistency allows for a plethora of new particles at the ≲ O(10) TeV scale, hence accessible to future collider and low-energy experiments.
dc.languageen
dc.publisherSpringer Science and Business Media Deutschland GmbH
dc.rightshttps://link.springer.com/article/10.1007/JHEP03(2022)034#rightslink
dc.rightsAttribution 4.0 International (CC BY 4.0)
dc.subjectBeyond Standard Model
dc.subjectGauge Symmetry
dc.subjectNeutrino Physics
dc.subjectLeptons
dc.subjectGauge Group
dc.subjectScalar
dc.titleScotogenic neutrino masses with gauged matter parity and gauge coupling unification
dc.typeArtículo


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