Scalar Dark Matter, GUT baryogenesis and Radiative neutrino mass
arXiv:1806.08204 · doi:10.1103/PhysRevD.98.075024
Abstract
We investigate an interesting correlation among dark matter phenomenology, neutrino mass generation and GUT baryogenesis, based on the scotogenic model. The model contains additional right-handed neutrinos and a second Higgs doublet , both of which are odd under an imposed symmetry. The neutral component of , i.e. the lightest of the -odd particles, is the dark matter candidate. Due to a Yukawa coupling involving , and the Standard Model leptons, the lepton asymmetry is converted into the dark matter asymmetry so that a non-vanishing asymmetry can arise from -conserving GUT baryogenesis, leading to a nonzero baryon asymmetry after the sphalerons decouple. On the other hand, can also generate neutrino masses radiatively. In other words, the existence of as the dark matter candidate resuscitates GUT baryogenesis and realizes neutrino masses.
16 pages, 6 figures. v2: version accepted by PRD
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- Fermion Dark Matter with Leptogenesis in Minimal Scotogenic Model
- TeV Scale Leptogenesis with Dark Matter in Non-standard Cosmology
- Low-scale leptogenesis assisted by a real scalar singlet
- Observable Gravitational Waves in Minimal Scotogenic Model
- One-loop Matching of Scotogenic Model onto Standard Model Effective Field Theory up to Dimension 7