Solar neutrinos - Eclipse effect

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dc.creatorNarayan, Mohan
dc.creatorRajasekaran, G.
dc.creatorSinha, Rahul
dc.date1997-03-07
dc.date1997-03-12
dc.date.accessioned2026-07-07T08:58:25Z
dc.date.available2026-07-07T08:58:25Z
dc.descriptionIt 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.
dc.description16 Pages Revtex, 5 figures as one ps file. Typos corrected
dc.identifierhttps://arxiv.org/abs/astro-ph/9703044
dc.identifierhttp://arxiv.org/abs/astro-ph/9703044
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/147320
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.titleSolar neutrinos - Eclipse effect
dc.typetext

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