Neutrino mass, Dark Matter and Baryon Asymmetry via TeV-Scale Physics without Fine-Tuning - INSPIRE

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Neutrino mass, Dark Matter and Baryon Asymmetry via TeV-Scale Physics without Fine-Tuning

Jul, 2008

4 pages

Published in:

Phys.Rev.Lett. 102 (2009) 051805

e-Print:

0807.0361 [hep-ph]

DOI:

10.1103/PhysRevLett.102.051805

Report number:

UT-HET-011,
IFT-UAM-CSIC-08-40

View in:

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Abstract: (arXiv)

We propose an extended version of the standard model, in which neutrino oscillation, dark matter, and baryon asymmetry of the Universe can be simultaneously explained by the TeV-scale physics without assuming unnatural hierarchy among the mass scales. Tiny neutrino masses are generated at the three loop level due to the exact

Z_2

symmetry, by which 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.

14.60.Pq
12.60.Fr
14.80.Cp
neutrino: oscillation
neutrino: mass generation
dark matter: lifetime
baryon: asymmetry
symmetry: Z(2)
Higgs particle: multiplet
doublet: 2

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