Bi-Maximal Neutrino Mixing in SO(10)_{GUT}

Abstract

We find a grand unified SO(10) model which accommodates the bi-maximal neutrino mixing for vacuum-oscillation solutions to the atmospheric and the solar neutrino problems. This model maintains the original SO(10) mass relation between neutrino and up-type quark masses, $m_{{\nu }_2}/m_{{\nu }_3}\sim (m_c/m_t{)}^2$.

9 pages, Latex

References in corpus (2)

• Bi-Maximal Mixing of Three Neutrinos
• Large Lepton Mixing in a Coset-space Family Unification on $E_7/SU(5)\times U(1{)}^3$

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