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The Sudbury Neutrino Observatory

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arxiv nucl-ex/9910016 v2 pith:VJO3N6GR submitted 1999-10-25 nucl-ex astro-phhep-exhep-phphysics.ins-det

The SNO Collaboration This is my paper
classification nucl-exastro-phhep-exhep-phphysics.ins-det
keywords neutrinoobservatorysudburydetectorsolarcharged-cherenkovcomparison
verification ladder T0 review T1 audit T2 compute T3 formal
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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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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Neutrino Mass Predictions with an AI-based Algorithm under $A_4$ Modular Symmetry

    hep-ph 2025-08 reject novelty 3.0 of 10

    An A4 modular linear-seesaw neutrino model is fitted with the ILA optimizer, and the fitted parameters agree with oscillation and cosmological bounds.

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