Recent Results from the Sudbury Neutrino Observatory

Details Recent Results from the Sudbury Neutrino Observatory Recent Results from the Sudbury Neutrino Observatory

Apr 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005iche.conf..263d&link_type=abstract

HIGH ENERGY PHYSICS, ICHEP 2004. Proceedings of the 32nd International Conference. Held 16-22 August 2004 in Beijing, China. Edi

Physics

High Energy Physics

Scientific paper

The Sudbury Neutrino Observatory Collaboration (SNO) determined the total active (νx)8B solar neutrino flux to be 5.21±0.27(stat)±0.38(syst) × 106cm-2s-1, without assumptions about the energy dependence of the νe survival probability. Data from Phase I and II have been used to constrain the lifetime for nucleon decay to "invisible" modes, such as n → 3ν, and set limit on the electron antineutrino flux for the sun.

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