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      Sterile neutrino oscillations: the global picture

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          Review of Particle Physics

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            Direct Evidence for Neutrino Flavor Transformation from Neutral-Current Interactions in the Sudbury Neutrino Observatory

            Observations of neutral-current nu interactions on deuterium in the Sudbury Neutrino Observatory are reported. Using the neutral current (NC), elastic scattering, and charged current reactions and assuming the standard 8B shape, the nu(e) component of the 8B solar flux is phis(e) = 1.76(+0.05)(-0.05)(stat)(+0.09)(-0.09)(syst) x 10(6) cm(-2) s(-1) for a kinetic energy threshold of 5 MeV. The non-nu(e) component is phi(mu)(tau) = 3.41(+0.45)(-0.45)(stat)(+0.48)(-0.45)(syst) x 10(6) cm(-2) s(-1), 5.3sigma greater than zero, providing strong evidence for solar nu(e) flavor transformation. The total flux measured with the NC reaction is phi(NC) = 5.09(+0.44)(-0.43)(stat)(+0.46)(-0.43)(syst) x 10(6) cm(-2) s(-1), consistent with solar models.
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              Measurement of the Solar Electron Neutrino Flux with the Homestake Chlorine Detector

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                Author and article information

                Journal
                Journal of High Energy Physics
                J. High Energ. Phys.
                Springer Nature
                1029-8479
                May 2013
                May 10 2013
                May 2013
                : 2013
                : 5
                Article
                10.1007/JHEP05(2013)050
                285d2611-06c2-408b-9f04-8197a4c1af4f
                © 2013
                History

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