Neutral Current Detectors in the Sudbury Neutrino Observatory

Details Neutral Current Detectors in the Sudbury Neutrino Observatory Neutral Current Detectors in the Sudbury Neutrino Observatory

Mar 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004paun.conf..362s&link_type=abstract

PARTICLES AND THE UNIVERSE. Proceedings of the Eighteenth Lake Louise Winter Institute. Held 16-22 February 2003 in Lake Louise,

Physics

Scientific paper

The Sudbury Neutrino Observatory (SNO) is a heavy water solar neutrino Cherenkov detector with sensitivity to the neutral current, charged current, and elastic scattering reactions. The SNO experiment is poised to enter the neutral current detector (NCD) phase, during which 3He proportional counters will be deployed into the heavy water in order to detect neutrons liberated by the neutral current reaction. The NCD phase will provide a largely independent measurement of the total 8B solar neutrino flux as well as event-by-event discrimination between neutral current and charged current interactions in case of a supernova.

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