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arXiv · nucl-ex/9910016

The Sudbury Neutrino Observatory

The SNO Collaboration
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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.

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The SNO Collaboration. 1999-11-03. The Sudbury Neutrino Observatory. https://doi.org/10.1016/s0168-9002(99)01469-2

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