Prospects for a day-night 37Cl solar-neutrino oscillation experiment

Details Prospects for a day-night 37Cl solar-neutrino oscillation experiment Prospects for a day-night 37Cl solar-neutrino oscillation experiment

Dec 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987phrvd..36.3571c&link_type=abstract

Physical Review D (Particles and Fields), Volume 36, Issue 12, 15 December 1987, pp.3571-3574

Physics

18

Quark And Lepton Masses And Mixing

Scientific paper

If neutrino oscillations in the solar interior are responsible for the suppressed 8B solar-neutrino flux measured by the Homestake 37Cl detector, then for certain values of neutrino mass difference and mixing angle, distinct day-night differences in the counting rate are expected due to propagation effects in the Earth. We describe the plans to measure day-night variations with the 37Cl detector, and present the results of calculations of 37Cl detector sensitivity and expected results.

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