Time-Variations of Solar Neutrino Signals

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dc.creatorKrastev, P. I.
dc.date1996-10-13
dc.date.accessioned2026-07-07T04:00:27Z
dc.date.available2026-07-07T04:00:27Z
dc.descriptionThe most popular solutions of the solar neutrino problem which assume massive neutrinos predict varying with time signals in the solar neutrino detectors. The variations represent a distinctive feature of these solutions and do not depend on the theoretically predicted total flux of neutrinos from the Sun. The sensitivity of SuperKamiokande and SNO to day-night variations due to regeneration in the Earth is estimated.
dc.description4 pages, 2 figures, LATEX, uses sprocl.sty (included) talk presented at the DPF '96 meeting, Minneapolis, MN, August 10 - 15, 1996
dc.identifierhttps://arxiv.org/abs/hep-ph/9610339
dc.identifierhttp://arxiv.org/abs/hep-ph/9610339
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/46560
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.titleTime-Variations of Solar Neutrino Signals
dc.typetext

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