A See-Saw Model for Atmospheric and Solar Neutrino Oscillations
arXiv:hep-ph/9810309 · doi:10.1016/S0370-2693(98)01395-1
Abstract
We have constructed an explicit see-saw model containing two singlet neutrinos, one carrying a gauge charge with an intermediate mass scale of GeV along with a sterile one near the GUT (grand unification theory) scale of GeV. With these mass scales and a reasonable range of Yukawa couplings, the model can naturally account for the near-maximal mixing of atmospheric neutrino oscillations and the small mixing matter-enhanced oscillation solution to the solar neutrino deficit.
10 pages latex file; Minor changes (to be published in Phys Lett B)
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