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arXiv · hep-ph/9209214

From Fermion Mass Matrices to Neutrino Oscillations

K. S. Babu·Q. Shafi
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Abstract

We present an ansatz for the quark and lepton mass matrices, derivable from SO(10) type GUTs, which accommodates a heavy $(> 92 GeV)$ top quark and permits large mixings in the $ν_μ\leftrightarrow ν_τ$ sector (as suggested by the recent Kamiokande and IMB data on the atmospheric neutrinos). The well known asymptotic relations $m_b = m_τ$, $m_s = \frac{1}{3} m_μ$ and $m_dm_s = m_e m_μ$ all hold to a good approximation. Depending on $ν_μ\leftrightarrow ν_τ$ mixing which can even be maximal, the mixing angle relevant for solar neutrino oscillation lies in the range $7.8 \times 10^{-3} \stackrel{_<}{_\sim} \sin^2 2θ_{eμ} \stackrel{_<}{_\sim} 2.1 \times 10^{-2}$. For the $^{71}$Ga experiment the event rate, normalized against the standard solar model prediction of 132 SNU, is estimated to be between 80 and 20 SNU.

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K. S. Babu, Q. Shafi. 1992-09-04. From Fermion Mass Matrices to Neutrino Oscillations. https://doi.org/10.1016/0370-2693(92)90688-z

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