Constraints On Radiative Neutrino Mass Models From Oscillation Data

Abstract

The three neutrino Zee model and its extension including three active and one sterile species are studied in the light of new neutrino oscillation data. We obtain analytical relations for the mixing angle in solar oscillations in terms of neutrino mass squared differences. For the four neutrino case, we obtain the result $\mathsf{si}{\mathsf{n}}^{2}2{\theta }_{\odot }\approx 1-[(\mathsf{\Delta }{\mathsf{m}}_{\mathsf{Atm}}^2{)}^2/(4\Delta {\mathsf{m}}_{\mathsf{LSND}}^2\mathsf{\Delta }{\mathsf{m}}_{\odot }^2){]}^2$, which can accommodate both the large and small mixing scenarios. We show that within this framework, while both the SMA-MSW and the LMA-MSW solutions can easily be accommodated, it would be difficult to reconcile the LOW-QVO solutions. We also comment on the active-sterile admixture within phenomenologically viable textures.

The paper has been substantially rewritten, especially in Section IV, though the basic results are unchanged. Some new references and an appendix have been added

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Cited by in corpus (5)

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• Bilarge Neutrino Mixing and μ- τPermutation Symmetry for Two-loop Radiative Mechanism
• Constraining Mass Spectra with Sterile Neutrinos from Neutrinoless Double Beta Decay, Tritium Beta Decay and Cosmology
• Escape from washing out of baryon number in a two-zero-texture general Zee model compatible with the large mixing angle MSW solution
• A minimal three generation seesaw scenario for LSND