THE SOLAR NEUTRINO PROBLEM
arXiv:hep-ph/9503430 · doi:10.1146/annurev.aa.33.090195.002331
Abstract
The solar neutrino problem has persisted for almost three decades. Recent results from Kamiokande, SAGE, and GALLEX indicate a pattern of neutrino fluxes that is very difficult to reconcile with plausible variations in standard solar models. This situation is reviewed and suggested particle physics solutions are discussed. A summary is given of the important physics expected from SNO, SuperKamiokande, and other future experiments.
66 pages, LATEX, 18 figures available by mail on request