The solar neutrino deficit: Principle and interest (a modern problem)

Details The solar neutrino deficit: Principle and interest (a modern problem) The solar neutrino deficit: Principle and interest (a modern problem)

Jan 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995stin...9631509r&link_type=abstract

Conference Paper, International Conference on the Structure of Baryons Dept. of Physics.

Mathematics

Probability

Light Elements, Luminosity, Neutrinos, Oscillations, Probability Theory, Stability, Sun

Scientific paper

Sufficient data now exist that tests, independent of any solar model, can be made of whether solar neutrino experiment are consistent with the minimal Standard Model (stable, massless neutrinos). If the experimental uncertainties are correctly estimated and the sun is generating energy by light-element fusion in quasi-static equilibrium, the probability of a standard-physics solution is less than 1.2%. Even when the luminosity constraint is abandoned, the probability is not more than 5%. The sensitivity of the conclusions to input parameters is explored. New experiments nearing completion (SNO and SuperKamiokande) are expected to provide decisive evidence of neutrino oscillations, if they are indeed the explanation.

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