Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientific paper
1999-08-10
Phys.Rev. D60 (1999) 073006
Physics
High Energy Physics
High Energy Physics - Phenomenology
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.
Burgess Cliff P.
Narayan Mohan
Rajasekaran Guruswamy
Sinha Rahul
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