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The Sudbury Neutrino Observatory

Abstract:
The Sudbury Neutrino Observatory is a second-generation water Cherenkov detector designed to determine whether the currently observed solar neutrino deficit is a result of neutrino oscillations. The detector is unique in its use of D2O as a detection medium, permitting it to make a solar model-independent test of the neutrino oscillation hypothesis by comparison of the charged- and neutral-current interaction rates. In this paper the physical properties, construction, and preliminary operation of the Sudbury Neutrino Observatory are described. Data and predicted operating parameters are provided whenever possible.
Publication status:
Published

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Publisher copy:
10.1016/S0168-9002(99)01469-2

Authors



Publisher:
Elsevier
Journal:
NUCLEAR INSTRUMENTS and METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT More from this journal
Volume:
449
Issue:
1-2
Pages:
172-207
Publication date:
2000-07-11
DOI:
ISSN:
0168-9002


Language:
English
Keywords:
Pubs id:
pubs:11191
UUID:
uuid:9cf2e27c-ee89-4878-9682-8390d6321f6f
Local pid:
pubs:11191
Source identifiers:
11191
Deposit date:
2012-12-19

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