Neutrino Mass, Dark Matter and Baryon Asymmetry via Tev-Scale Physics

Details Neutrino Mass, Dark Matter and Baryon Asymmetry via Tev-Scale Physics Neutrino Mass, Dark Matter and Baryon Asymmetry via Tev-Scale Physics

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010dmap.conf..170a&link_type=abstract

DARK MATTER IN ASTROPHYSICS AND PARTICLE PHYSICS . Proceedings of the 7th International Heidelberg Conference on Dark 2009 . Hel

Astronomy and Astrophysics

Astrophysics

Scientific paper

We discuss a TeV-scale model, in which neutrino masses and mixings, dark matter, and baryon asymmetry of the Universe can be simultaneously explained without assuming large hierarchy among the mass scales. Imposing the exact Z2 symmetry, tiny neutrino masses are generated at the three loop level and stability of the dark matter candidate is guaranteed. Moreover the necessary conditions for the electroweak baryogenesis are satisfied via the extended Higgs sector. The model provides a distinctive experimental signature especially in Higgs phenomenology and dark matter physics.

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