Journal
NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT
Volume 489, Issue 1-3, Pages 178-188Publisher
ELSEVIER SCIENCE BV
DOI: 10.1016/S0168-9002(02)00860-4
Keywords
Sudbury Neutrino Observatory; solar neutrinos; radioactive source; energy calibration; Cherenkov detector; event reconstruction; gas transport; 8B spectrum
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A calibration source employing Li-8 (t(1/2) = 0.838 s) has been developed for use with the Sudbury Neutrino Observatory (SNO). This source creates a spectrum of beta-particles with an energy range similar to that of the SNO B-8 solar neutrino signal. The source is used to test the SNO detector's energy response. position reconstruction and data reduction algorithms. The Li-8 isotope is created using a deuterium-tritium neutron generator in conjunction with a B-11 target, and is carried to a decay chamber using a gas, aerosol transport system. The decay chamber detects prompt alpha-particles by gas scintillation in coincidence with the beta-particles which exit through a thin stainless steel wall. A description is given of the production, transport, and tagging techniques along with a discussion of the performance and application of the source. (C) 2002 Elsevier Science B.V. All rights reserved.
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