On the Day-Night Effect and CC to NC Event Rate Ratio Predictions for the SNO Detector

Details On the Day-Night Effect and CC to NC Event Rate Ratio Predictions for the SNO Detector On the Day-Night Effect and CC to NC Event Rate Ratio Predictions for the SNO Detector

2002-01-11

arxiv.org/abs/hep-ph/0201087v3

Phys.Lett. B534 (2002) 17-27

Physics

High Energy Physics

High Energy Physics - Phenomenology

16 pages, LATEX; 10 pages of text, 12 eps-files; the text includes 6 figures; results and conclusions unchanged, the iso-(D-N)

Scientific paper

10.1016/S0370-2693(02)01544-7

Detailed predictions for the D-N asymmetry for the Super-Kamiokande and SNO experiments, as well as for the ratio of the CC and NC event rates measured by SNO, in the cases of the LMA MSW and of the LOW solutions of the solar neutrino problem, are derived. The possibilities to further constrain the regions of the LMA MSW and LOW solutions of the solar neutrino problem by using the forthcoming SNO data on the D-N asymmetry and on the CC to NC event rate ratio are also discussed.

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