Prospects for a day-night Cl37 solar-neutrino oscillation experiment
If neutrino oscillations in the solar interior are responsible for the suppressed B8 solar-neutrino flux measured by the Homestake Cl37 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 Cl37 detector, and present the results of calculations of Cl37 detector sensitivity and expected results. © 1987 The American Physical Society.
Publication Source (Journal or Book title)
Physical Review D
Cherry, M., & Lande, K. (1987). Prospects for a day-night Cl37 solar-neutrino oscillation experiment. Physical Review D, 36 (12), 3571-3574. https://doi.org/10.1103/PhysRevD.36.3571