PREDICTING THE NEUTRINO SPECTRUM IN SUSY SO(10)

We present a systematic search for SUSY SO(10) models which predict th e neutrino properties. The models are based on the five sets of quark mass matrices, with texture zeros, discussed recently by Roberts, Ramo nd and Ross. We found 8 such neutrino textures three of which can solv e the solar neutrino problem. The latter have tau-neutrino masses of f ew eV i.e. relevant for cosmology and nu(tau)-nu(mu) mixing angles tha t can be observed by the CHORUS, NOMAD and P803 experiments.