Models of Neutrino Masses and Baryogenesis
arXiv:hep-ph/9906335 · doi:10.1007/s12043-000-0010-8
Abstract
Majorana masses of the neutrino implies lepton number violation and is intimately related to the lepton asymmetry of the universe, which gets related to the baryon asymmetry of the universe in the presence of the sphalerons during the electroweak phase transition. Assuming that the baryon asymmetry of the universe is generated before the electroweak phase transition, it is possible to dicriminate different classes of models of neutrino masses. While see-saw mechanism and the triplet higgs mechanism are preferred, the Zee-type radiative models and the R-parity breaking models requires additional inputs to generate baryon asymmetry of the universe during the electroweak phase transition.
27 pages including 5 figures; Review article for Pramana: the Indian Journal of Physics
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- Adjoint bulk scalars and supersymmetric unification in the presence of extra dimensions
- Developments in high energy theory