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      FLUX OF ATMOSPHERIC NEUTRINOS

      1 , 2 , 1 , 2
      Annual Review of Nuclear and Particle Science
      Annual Reviews

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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 Rate of\({\nu }_{e}+\mathit{d}\to \mathit{p}+\mathit{p}+{\mathit{e}}^{-}\)Interactions Produced by\({}_{}{}^{8}{}_{}{}^{}B\)Solar Neutrinos at the Sudbury Neutrino Observatory

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              Solar Modulation of Galactic Cosmic Rays

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                Author and article information

                Journal
                Annual Review of Nuclear and Particle Science
                Annu. Rev. Nucl. Part. Sci.
                Annual Reviews
                0163-8998
                1545-4134
                December 2002
                December 2002
                : 52
                : 1
                : 153-199
                Affiliations
                [1 ]Bartol Research Institute, University of Delaware, Newark, Delaware 19716; e-mail:
                [2 ]Institute for Cosmic Ray Research, University of Tokyo, 5-1-5 Kashiwanoha Kashiwa-shi, Chiba 277-8582, Japan; e-mail:
                Article
                10.1146/annurev.nucl.52.050102.090645
                cedc8014-8b87-4aad-9f9b-3491cb77f42f
                © 2002
                History

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