  A recent experiment LSND at Los Alamos has provided\cite{1} an indication of
$\overline{\nu}_{\mu} - \overline{\nu}_e$ oscillations with $\Delta m^2$ of
order 1ev$^2$ or greater and $\sin^2 2 \theta_{e \mu}$ between $2 \times
10^{-3}$ and $10^{2}$. Such a value of $\Delta m^2$ for $\nu_{\mu} - \nu_e$
oscillations was not expected in the standard see-saw model\cite{2} suggested
by SO(10) with a large mass hierarchy because it leads to too large a value of
$m(\nu_{\tau})$ to fit cosmological constraints. Furthermore within that model
the LSND result is inconsistent with the indications of oscillations from both
atmospheric neutrinos\cite{3} and solar neutrinos.\cite{4}
