Bi-maximal Neutrino Mixing Pattern Reexamined
arXiv:hep-ph/9909514 · doi:10.1103/PhysRevD.61.057301
Abstract
I propose a simple extension of the bi-maximal neutrino mixing pattern, allowing slight coupling between solar and atmospheric neutrino oscillations as well as large CP violation. The new scenario is compatible with either the vacuum oscillation solution or the large-angle MSW solution to the solar neutrino
RevTex 6 pages. Minor changes. Phys. Rev. D (in press)
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