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THE SOLAR NEUTRINO PROBLEM
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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.
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Cited by 1 Pith paper
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The Gallium Solar Neutrino Capture Cross Section Revisited
Updated 71Ga solar neutrino capture cross sections raise the 8B and hep rates by about 7% and 10% over Bahcall's 1997 values and cut the uncertainties by a factor of 2 to 3.
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