Neutrino mass, dark matter, and Baryon asymmetry via TeV-scale physics without fine-tuning.
We propose an extended version of the standard model, in which neutrino oscillation, dark matter, and the baryon asymmetry of the Universe can be simultaneously explained by the TeV-scale physics without assuming a large hierarchy among the mass scales. Tiny neutrino masses are generated at the three-loop level due to the exact Z2 symmetry, by which the stability of the dark matter candidate is guaranteed. The extra Higgs doublet is required not only for the tiny neutrino masses but also for successful electroweak baryogenesis. The model provides discriminative predictions especially in Higgs phenomenology, so that it is testable at current and future collider experiments.
Aoki
Mayumi
M
ICRR, University of Tokyo, Kashiwa 277-8582, Japan.
Kanemura
Shinya
S
Seto
Osamu
O