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SO(10) and Large numu - nutau Mixing

S. M. Barr, C. H. Albright

hep-pharXiv:hep-ph/0001052

Abstract

A general approach to understanding the large mixing seen in atmospheric neutrinos is explained, as well as a highly predictive SO(10) model which implements this approach. It is also seen how bimaximal mixing naturally arises in this scheme. (Talk presented at NNN99, SUNY Stony Brook, Sept. 22-26, 1999)

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