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arXiv · hep-ph/0001052

SO(10) and Large nu_mu - nu_tau Mixing

S. M. Barr·C. H. Albright
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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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S. M. Barr, C. H. Albright. 2000-01-06. SO(10) and Large nu_mu - nu_tau Mixing. https://doi.org/10.1063/1.1361726

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