Simple theory for scotogenic dark matter with residual matter-parity
A. E. C\'arcamo Hern\'andez, Jos\'e W. F. Valle, Carlos A., Vaquera-Araujo
TL;DR
This paper introduces a minimal theoretical model where dark matter stability arises from residual matter-parity after symmetry breaking, linking dark sector particles to an extended gauge symmetry.
Contribution
It presents the simplest scotogenic dark matter model based on the original SVS theory, providing a natural origin for dark sector particles and matter-parity.
Findings
Dark matter stability from residual matter-parity
Natural origin of dark sector particles in the model
Simplest realization of scotogenic dark matter
Abstract
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.
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