Solar neutrino flux measurement from the pure D2O-phase of the sudbury neutrino observatory

Details Solar neutrino flux measurement from the pure D2O-phase of the sudbury neutrino observatory Solar neutrino flux measurement from the pure D2O-phase of the sudbury neutrino observatory

May 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003nupha.718...75c&link_type=abstract

Nuclear Physics A, Volume 718, p. 75-82.

Physics

Nuclear Physics

Scientific paper

The measured non-νe active component of the solar neutrino flux from the pure-D2O phase (at 5 MeV threshold) is 3.41-0.45+0.45(stat.)-0.45+0.48 (syst.) × 106 cm-2s-1, 5.3σ greater than zero. This provides a strong model independent evidence for solar νe flavor transformation. The measured total flux, φNC, is consistent with solar models. A global MSW study based on SNO day-night spectra and existing data strongly favors the LMA region.
Supported by DOE Contract No. DE-AC03-76SF00098

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