An Experimentalist's Overview of Solar Neutrinos

Details An Experimentalist's Overview of Solar Neutrinos An Experimentalist's Overview of Solar Neutrinos

Feb 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012jphcs.337a2056o&link_type=abstract

Journal of Physics: Conference Series, Volume 337, Issue 1, pp. 012056 (2012).

Physics

Scientific paper

Four decades of solar neutrino research have demonstrated that solar models do a remarkable job of predicting the neutrino fluxes from the Sun, to the extent that solar neutrinos can now serve as a calibrated neutrino source for experiments to understand neutrino oscillations and mixing. In this review article I will highlight the most significant experimental results, with emphasis on the latest model-independent measurements from the Sudbury Neutrino Observatory. The solar neutrino fluxes are seen to be generally well-determined experimentally, with no indications of time variability, while future experiments will elucidate the lower energy part of the neutrino spectrum, especially pep and CNO neutrinos.

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