K. Ishihara

Measurement of neutrino oscillation with KamLAND: Evidence of spectral distortion

We present results of a study of neutrino oscillation based on a 766 ton-year exposure of KamLAND to reactor anti-neutrinos. We observe 258 \nuebar\ candidate events with energies above 3.4 MeV compared to 365.2 events expected in the absence of neutrino oscillation. Accounting for 17.8 expected background events, the statistical significance for reactor \nuebar disappearance is 99.998%. The observed energy spectrum disagrees with the expected spectral shape in the absence of neutrino oscillation at 99.6% significance and prefers the distortion expected from \nuebar oscillation effects. A two-neutrino oscillation analysis of the KamLAND data gives \DeltaMSq = 7.9

Measurement of the flux and zenith angle distribution of upward through going muons in Kamiokande II + III

^{+0.6}_{-0.5}\times10^{-5}

Study of neutron background in the atmospheric neutrino sample in Kamiokande

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Self-shielding effect of a single phase liquid xenon detector for direct dark matter search

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SOLAR NEUTRINO DATA COVERING SOLAR CYCLE 22

. A global analysis of data from KamLAND and solar neutrino experiments yields \DeltaMSq = 7.9

Large scale anisotropy of the cosmic ray muon flux in Kamiokande

^{+0.6}_{-0.5}\times10^{-5}

Publisher's Note: Search for dark matter WIMPs using upward through-going muons in Super-Kamiokande [Phys. Rev. D 70, 083523 (2004)]

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High Sensitivity Search for ν̄e's from the Sun and Other Sources at KamLAND

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Experimental study of high-energy atmospheric neutrinos in Kamiokande

and \ThetaParam = 0.40