1996/10/13 by P. I. Krastev, Krastev, P. I.
Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #High Energy Physics - Phenomenology (hep-ph) #astro-ph #hep-ph
paper · pdf · doi:10.48550/arxiv.hep-ph/9610339
4 pages, 2 figures, LATEX, uses sprocl.sty (included) talk presented at the DPF '96 meeting, Minneapolis, MN, August 10 - 15, 1996
arxiv created 1996/10/13 · arxiv updated 2009/11/30
The 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.