Cosmological implications of a class of SO(10) models
arXiv:hep-ph/9705212 · doi:10.1016/0920-5632(96)00260-5
Abstract
The cosmological implications of a class of SO(10) models are discussed. In particular we show how a good prediction for neutrino masses is obtained in order to fit with the MSW mechanism to explain the solar neutrino flux deficit and with the predicted amount of the dark matter hot component. A possible scenario for baryogenesis is also considered.
latex file, 3 pages, appeared in Proceedings of TAUP 95, Toledo, 17 -21 September 1995. Nucl. Phys. B (Proc. Suppl.) 48 (1996) 272, Eds. A. Morales, J. Morales and J. A. Villar