Solar neutrinos - Eclipse effect
classification
🌌 astro-ph
hep-ph
keywords
neutrinoenhancementsolareclipseparametersborexinocalculatedcase
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It is pointed out that the enhancement of the solar neutrino rate in a real time detector like Super-Kamioka, SNO or Borexino due to neutrino oscillations in the moon during a partial or total solar eclipse may be observable. 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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