Journal article
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
Actions
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
Terms of use
- Copyright date:
- 2000
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