Solar Neutrinos and the Eclipse Effect

Physics – High Energy Physics – High Energy Physics - Phenomenology

Scientific paper

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24 Pages Revtex, 8 figures as one ps file. To appear in Phys. Rev. D; Some typos corrected and a reference added

Scientific paper

10.1103/PhysRevD.60.073006

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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