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Measurement of the Total Active 8B Solar Neutrino Flux at the Sudbury Neutrino Observatory with Enhanced Neutral Current Sensitivity

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arxiv nucl-ex/0309004 v1 pith:AYUTVP77 submitted 2003-09-06 nucl-ex hep-ex

SNO Collaboration This is my paper · ORCID
classification nucl-exhep-ex
keywords neutrinosolarfluxactivemeasurementsobservatorysensitivitystandard
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The Sudbury Neutrino Observatory (SNO) has precisely determined the total active (nu_x) 8B solar neutrino flux without assumptions about the energy dependence of the nu_e survival probability. The measurements were made with dissolved NaCl in the heavy water to enhance the sensitivity and signature for neutral-current interactions. The flux is found to be 5.21 +/- 0.27 (stat) +/- 0.38 (syst) x10^6 cm^{-2}s^{-1}, in agreement with previous measurements and standard solar models. A global analysis of these and other solar and reactor neutrino results yields Delta m^{2} = 7.1^{+1.2}_{-0.6}x10^{-5} ev^2 and theta = 32.5^{+2.4}_{-2.3} degrees. Maximal mixing is rejected at the equivalent of 5.4 standard deviations.

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Cited by 2 Pith papers

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

  1. Estimating amplitude of matter density fluctuations in solar and supernova models using neutrino flavor evolution

    astro-ph.HE 2026-07 conditional novelty 5.0 of 10

    SDA recovers density-fluctuation amplitudes from boundary neutrino flavor data in simplified solar and CCSN models, more reliably for the Sun and at high noise in CCSN.

  2. Probing Type II Seesaw Leptogenesis Through Lepton Flavor Violation

    hep-ph 2025-01 conditional novelty 4.0 of 10

    A scan over 3σ neutrino parameters yields the most conservative lower bounds on the triplet-Higgs cubic coupling from μ→eγ, μ→3e, and μ-e conversion.

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