Leptonic Fritzsch Matrices and Neutrino Oscillations

Abstract

It was recently shown by the authors that the Fritzsch ansatz for the quark mass matrices prescribed at the supersymmetric grand unified scale is compatible with a moderately heavy top quark ($m_t\simeq 120-150GeV$). Here we extend the ansatz to incorporate the charged leptons and the neutrinos. It is found that the ${\nu }_e-{\nu }_{\mu }$ mixing angle is small and consistent with the MSW solution of the solar neutrino puzzle. Furthermore, the model predicts observable ${\nu }_{\mu }-{\nu }_{\tau }$ oscillations with sin${}^{2}2{\theta }_{\mu \tau }\simeq 0.1$ and ${\nu }_{\tau }$ mass in the $(1-3)eV$ range.

15 pages in LaTeX, one figure avialable on request, BA-93-09

References in corpus (3)

• From Fermion Mass Matrices to Neutrino Oscillations
• Neutrino Masses in Flipped SU(5)
• Predictive Ansatz for Fermion Masses in SUSY GUTS

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