Neutral current and day night measurements from the pure D2O phase of SNO
The Sudbury Neutrino Observatory is a 1000 T D2O Cerenkov detector that is sensitive to B-8 solar neutrinos. The energy, radius, and direction with respect to the sun is Measured for each neutrino event; these distributions are used to separately determine the rates of the charged current, neutral c...
Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , |
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2003
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