6533b871fe1ef96bd12d0fb8

RESEARCH PRODUCT

An ultraviolet completion for the Scotogenic model

Pablo EscribanoAvelino VicenteAvelino Vicente

subject

PhysicsNuclear and High Energy PhysicsParticle physicsPhysicsQC1-999Scalar (mathematics)Dark matterHigh Energy Physics::PhenomenologyFOS: Physical sciencesContext (language use)ObservableParity (physics)Massless particleHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Goldstone bosonNeutrino

description

The Scotogenic model is an economical scenario that generates neutrino masses at the 1-loop level and includes a dark matter candidate. This is achieved by means of an ad-hoc $\mathbb{Z}_2$ symmetry, which forbids the tree-level generation of neutrino masses and stabilizes the lightest $\mathbb{Z}_2$-odd state. Neutrino masses are also suppressed by a quartic coupling, usually denoted by $\lambda_5$. While the smallness of this parameter is natural, it is not explained in the context of the Scotogenic model. We construct an ultraviolet completion of the Scotogenic model that provides a natural explanation for the smallness of the $\lambda_5$ parameter and induces the $\mathbb{Z}_2$ parity as the low-energy remnant of a global $\rm U(1)$ symmetry at high energies. The low-energy spectrum contains, besides the usual Scotogenic states, a massive scalar and a massless Goldstone boson, hence leading to novel phenomenological predictions in flavor observables, dark matter physics and colliders.

10.1016/j.physletb.2021.136717http://arxiv.org/abs/2107.10265