ILC phenomenology in a TeV scale radiative seesaw model for neutrino mass, dark matter and baryon asymmetry

Details ILC phenomenology in a TeV scale radiative seesaw model for neutrino mass, dark matter and baryon asymmetry ILC phenomenology in a TeV scale radiative seesaw model for neutrino mass, dark matter and baryon asymmetry

2010-08-14

arxiv.org/abs/1008.2407v1

Physics

High Energy Physics

High Energy Physics - Phenomenology

Prepared for the Proceedings of the ILC physics working group meetings, KEK

Scientific paper

We discuss phenomenology in a new TeV scale model which would explain neutrino oscillation, dark matter, and baryon asymmetry of the Universe simultaneously by the dynamics of the extended Higgs sector and TeV-scale right-handed neutrinos. Tiny neutrino masses are generated at the three-loop level due to the exact $Z_2$ symmetry, by which the stability of the dark matter candidate is guaranteed. The model provides various discriminative predictions in Higgs phenomenology, which can be tested at the Large Hadron Collider and the International Linear Collider.

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