Correlated Neutrino Oscillations
Abstract
In solar neutrino oscillations, if e has a significant third massive component, the allowed parameter space in m2 and 2 2 θ for the first two components is shown to be greatly increased. This third component may be correlated to atmospheric neutrino oscillations, as shown in a specific predictive seesaw model of the 3 × 3 neutrino mass matrix. Possible variations to include the recent LSND results are briefly discussed.
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