Pith. sign in

REVIEW 3 cited by

The Sudbury Neutrino Observatory

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 1602.02469 v2 pith:G2WKTZ43 submitted 2016-02-08 nucl-ex hep-exphysics.ins-det

A. Bellerive , J.R. Klein , A.B. McDonald , A.J. Noble , A.W.P. Poon (for the SNO Collaboration) This is my paper · ORCID
classification nucl-exhep-exphysics.ins-det
keywords neutrinosolarresultsactivedatadetectionexperimentflavors
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
abstract

This review paper provides a summary of the published results of the Sudbury Neutrino Observatory (SNO) experiment that was carried out by an international scientific collaboration with data collected during the period from 1999 to 2006. By using heavy water as a detection medium, the SNO experiment demonstrated clearly that solar electron neutrinos from $^8$B decay in the solar core change into other active neutrino flavors in transit to Earth. The reaction on deuterium that has equal sensitivity to all active neutrino flavors also provides a very accurate measure of the initial solar flux for comparison with solar models. This review summarizes the results from three phases of solar neutrino detection as well as other physics results obtained from analyses of the SNO data.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 3 Pith papers

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

  1. Fiber-coupled Digital Photo Sensors for Large Time Projection Chambers

    physics.ins-det 2025-02 conditional novelty 6.0 of 10

    A design concept that places fiber-coupled digital silicon photomultipliers inside the bulk of large liquid argon TPCs to capture prompt scintillation light for fast timing and particle identification.

  2. 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.

  3. Embeddings of the Standard Model in $E_8$

    hep-ph 2025-07 conditional novelty 5.0 of 10

    A modified E8 model puts the Standard Model inside the so(7,3) subalgebra with compact SU(3), and uses particle coordinates in four dimensions to compute several mixing angles and mass relations.

Pith tools