2003AIP conference proceedingsRequires access

Neutrino Experiments with Super-Kamiokande

Michael Smy

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Abstract

Super‐Kamiokande’s measurements of the solar and atmospheric neutrino flux yielded first evidence for oscillation of atmospheric vμ’s into vτ’s and (together with data from the SNO experiment) first evidence for oscillation of solar ve’s into vμ’s or vτ’s. Data from Super‐Kamiokande also constrained the neutrino mixing in both cases to be large. In Super‐Kamiokande, the flux and energy spectrum of the first long baseline accelerator vμ’s were measured, they favor neutrino oscillations consistent with the atmospheric neutrino analysis.

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Super‐Kamiokande’s measurements of the solar and atmospheric neutrino flux yielded first evidence for oscillation of atmospheric vμ’s into vτ’s and (together with data from the SNO experiment) first evidence for oscillation of solar ve’s into vμ’s or vτ’s. Data from Super‐Kamiokande also constrained the neutrino mixing in both cases to be large. In Super‐Kamiokande, the flux and energy spectrum of the first long baseline accelerator vμ’s were measured, they favor neutrino oscillations consistent with the atmospheric neutrino analysis.

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Available abstract

Super‐Kamiokande’s measurements of the solar and atmospheric neutrino flux yielded first evidence for oscillation of atmospheric vμ’s into vτ’s and (together with data from the SNO experiment) first evidence for oscillation of solar ve’s into vμ’s or vτ’s. Data from Super‐Kamiokande also constrained the neutrino mixing in both cases to be large. In Super‐Kamiokande, the flux and energy spectrum of the first long baseline accelerator vμ’s were measured, they favor neutrino oscillations consistent with the atmospheric neutrino analysis.

Key concepts: Super-Kamiokande, Solar neutrino, Physics, Neutrino oscillation, Neutrino, Solar neutrino problem, Flux (metallurgy), Particle physics

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