1995/07/03 by Ernest Ma, Ma, Ernest
Physics and Astronomy · #FOS: Physical sciences #High Energy Physics - Phenomenology (hep-ph) #hep-ph
paper · pdf · doi:10.48550/arxiv.hep-ph/9507209
6 pages, 1 figure not included, talk given at Valencia 95
arxiv created 1995/07/03 · arxiv updated 2009/11/30
In solar neutrino oscillations, if νe has a significant third massive component, the allowed parameter space in Δm2 and sin2 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.