6533b7cffe1ef96bd125874d

RESEARCH PRODUCT

Dark matter stability and Dirac neutrinos using only Standard Model symmetries

Salvador Centelles-chuliáRicardo CepedelloCesar BonillaCesar BonillaEduardo PeinadoRahul SrivastavaRahul Srivastava

subject

Physics010308 nuclear & particles physicsDark matterDirac (software)FOS: Physical sciencesComputer Science::Digital Libraries01 natural sciencesAction (physics)Symmetry (physics)ddc:Standard Model (mathematical formulation)Theoretical physicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesHomogeneous spaceAnomaly (physics)Neutrino010306 general physics

description

We provide a generic framework to obtain stable dark matter along with naturally small Dirac neutrino masses generated at the loop level. This is achieved through the spontaneous breaking of the global $U(1)_{B-L}$ symmetry already present in Standard Model. The $U(1)_{B-L}$ symmetry is broken down to a residual even $\mathcal{Z}_n$; $n \geq 4$ subgroup. The residual $\mathcal{Z}_n$ symmetry simultaneously guarantees dark matter stability and protects the Dirac nature of neutrinos. The $U(1)_{B-L}$ symmetry in our setup is anomaly free and can also be gauged in a straightforward way. Finally, we present an explicit example using our framework to show the idea in action.

10.1103/physrevd.101.033011http://arxiv.org/abs/1812.01599