Neutrino oscillations and mixings with three flavors
Tommy Ohlsson, Hakan Snellman
Abstract
Global fits to all data of candidates for neutrino oscillations are presented in the framework of a three-flavor model. The analysis excludes mass regions where the MSW effect is important for the solar neutrino problem. The best fit gives θ1 ≈ 28.9, θ2 ≈ 4.2, θ3 ≈ 45.0, m22 - m12 ≈ 2.87 · 10-4 eV2, and m32 - m22 ≈ 1.11 eV2 indicating essentially maximal mixing between the two lightest neutrino mass eigenstates.
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