Three Methods for Event - Type Identification in the SNO Detector
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ar X iv : h ep - p h / 01 02 28 8 v 1 2 3 Fe b 20 01 Solar neutrino event spectra : Tuning SNO to equalize Super - Kamiokande
The Super-Kamiokande (SK) and the Sudbury Neutrino Observatory (SNO) experiments are monitoring the flux of 8 B solar neutrinos through the electron energy spectrum from the reactions ν e,µ,τ + e − → ν e,µ,τ + e − and ν e + d → p + p+e − , respectively. We show that the SK detector response to 8 B neutrinos in each bin of the electron energy spectrum (above 8 MeV) can be approximated, with good...
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Detailed predictions for the D-N asymmetry for the Super-Kamiokande experiment, as well as for the Full Night and Core D-N asymmetries in the solar neutrino induced CC event rate and for the Day, Night and Core ratios of the CC and NC event rates, measured in the SNO experiment, are derived in the cases of the LMA MSW and LOW solutions of the solar neutrino problem. The indicated observables fo...
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