arXiv:hep-ph/0001052·v1·High Energy Physics — Phenomenology
SO(10) and Large nu_mu - nu_tau Mixing
S. M. Barr (Bartol)🇺🇸 · C. H. Albright (FNAL)🇺🇸
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)
Comments: 10 pages, LaTex