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

Preprint

11 January 2002

preprint
Published by arXiv in arXiv

Abstract

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.

Keywords

SOLAR NEUTRINO PROBLEM
EVENT RATE RATIO
NC EVENT RATE
EVENT RATES
RATE RATIO
ASYMMETRY
CC TO NC
LMA

All Related Versions

Version 1, 2002-01-11, ArXiv
Version 2, 2002-01-14, ArXiv
Version 3, 2002-04-21, ArXiv
Published version: Physics Letters B, 534 (1-4), 17.

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