0000000001110681

AUTHOR

A. E. Cárcamo Hernández

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Simple theory for scotogenic dark matter with residual matter-parity

2020

Dark matter stability can result from a residual matter-parity symmetry surviving spontaneous breaking of an extended gauge symmetry. We propose the simplest scotogenic dark matter completion of the original SVS theory (Phys.Rev. D22 (1980) 738), in which the "dark sector" particles as well as matter-parity find a natural theoretical origin in the model. We briefly comment on its main features.

PhysicsNuclear and High Energy Physics010308 nuclear & particles physicsDark matterFOS: Physical sciencesParity (physics)Astrophysics::Cosmology and Extragalactic AstrophysicsResidual01 natural scienceslcsh:QC1-999Theoretical physicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicslcsh:PhysicsGauge symmetry
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