SO(10) and Large nu_mu - nu_tau Mixing
arXiv:hep-ph/0001052 · doi:10.1063/1.1361726
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)
10 pages, LaTex