A See-Saw Model for Atmospheric and Solar Neutrino Oscillations

Physics – High Energy Physics – High Energy Physics - Phenomenology

Scientific paper

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10 pages latex file; Minor changes (to be published in Phys Lett B)

Scientific paper

10.1016/S0370-2693(98)01395-1

We have constructed an explicit see-saw model containing two singlet neutrinos, one carrying a $(B-3L_e)$ gauge charge with an intermediate mass scale of $\sim O(10^{10})$ GeV along with a sterile one near the GUT (grand unification theory) scale of $\sim O(10^{16})$ 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.

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