1997/05/27 by S. M. Bilenky, Bilenky, S. M., C. Giunti +3
Physics and Astronomy · #FOS: Physical sciences #High Energy Physics - Phenomenology (hep-ph) #hep-ph
paper · pdf · doi:10.48550/arxiv.hep-ph/9705436
19 pages including 5 figures, Latex2e. Talk presented by S. M. Bilenky at the Fourth International Solar Neutrino Conference, Heidelberg, Germany, April 8-11, 1997
arxiv created 1997/05/27 · arxiv updated 2009/11/30
What information about the neutrino mass spectrum and mixing matrix can be inferred from the existing neutrino oscillation data? We discuss here the answer to this question in the case of mixing of three and four neutrinos. We present the constraints on the effective Majorana mass <m> that can be obtained from the results of reactor neutrino oscillation experiments and from atmospheric neutrino data. We discuss the bounds on the oscillation probabilities in long-baseline neutrino oscillation experiments that follow from the results of short-baseline experiments. Some remarks on a model-independent approach to the solar neutrino problem are also made.