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arXiv · hep-ph/9908313

Solar Neutrinos and the Eclipse Effect

Mohan Narayan·G. Rajasekaran·Rahul Sinha·C. P. Burgess
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Abstract

The solar neutrino counting rate in a real time detector like Super--Kamiokanda, SNO, or Borexino is enhanced due to neutrino oscillations in the Moon during a partial or total solar eclipse. The enhancement is calculated as a function of the neutrino parameters in the case of three flavor mixing. This enhancement, if seen, can further help to determine the neutrino parameters.

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Mohan Narayan, G. Rajasekaran, Rahul Sinha, C. P. Burgess. 1999-09-01. Solar Neutrinos and the Eclipse Effect. https://doi.org/10.1103/physrevd.60.073006

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