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A See-Saw Model for Atmospheric and Solar Neutrino Oscillations
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abstract
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.
Forward citations
Cited by 2 Pith papers
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A Minimal Dark $SU(2)$ Origin of a Massless Dirac Neutrino
A minimal dark SU(2)_D model with anomaly cancellation and Z4 symmetry generates a rank-two Dirac neutrino mass matrix enforcing one exactly massless neutrino.
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Confronting the seesaw mechanism with neutrino oscillations: a general and explicit analytical bridge
The paper provides, for the first time, explicit analytical expressions for the two mass-squared differences, three mixing angles, and effective Dirac CP phase of the canonical seesaw mechanism in terms of its 18 para...
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