Signals, backgrounds and calibrations in the Sudbury Neutrino Observatory

Details Signals, backgrounds and calibrations in the Sudbury Neutrino Observatory Signals, backgrounds and calibrations in the Sudbury Neutrino Observatory

Jul 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995aipc..338..893s&link_type=abstract

The 5th conference on the intersections of particle and nuclear physics. AIP Conference Proceedings, Volume 338, pp. 893-900 (1

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Neutrino, Muon, Pion, And Other Elementary Particles, Cosmic Rays, Neutrino, Muon, Pion, And Other Elementary Particle Detectors, Cosmic Ray Detectors

Scientific paper

The Sudbury Neutrino Observatory is a large underground neutrino detector which is presently under construction, at a depth of 6800 ft, near Sudbury, Canada. This heavy water detector is designed to study neutrinos from the sun and from other sources with spectral resolution, high counting rates and extremely low backgrounds. The detector and the expected signals from it are discussed in this paper. The important ancillary measurements of backgrounds and detector calibration are outlined.

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