'Super kamiokande' diaporamas de présentation

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Neutrino Ocillations and Astroparticle Physics (2)

Neutrino Ocillations and Astroparticle Physics (2). John Carr Centre de Physique des Particules de Marseille (IN2P3/CNRS). Pisa, 7 May 2002. ? Neutrino Oscillations - Solar Neutrinos - Atmospheric Neutrinos

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Neutrino Ocillations and Astroparticle Physics (2)

Neutrino Ocillations and Astroparticle Physics (2). John Carr Centre de Physique des Particules de Marseille (IN2P3/CNRS). Pisa, 7 May 2002. ? Neutrino Oscillations - Solar Neutrinos - Atmospheric Neutrinos

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Neutrino Physics

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Super Beam Experiments

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Super-KamiokaNDE (Universe, Mankind and Neutrinos)

Super-KamiokaNDE (Universe, Mankind and Neutrinos). 2008-09-05 at Erice. Abstract :

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Neutrino Physics

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Recent Results from Neutrino Experiments and Plans for the Neutrino Super Beam in Japan

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Shin-ichi Kurokawa KEK ACAT03 Tsukuba, Japan December 1, 2003

Overview of KEK Activities. Shin-ichi Kurokawa KEK ACAT03 Tsukuba, Japan December 1, 2003. Accelerators in KEK. TRISTAN. KEKB. K2K. AR. 12-GeV PS. Photon Factory. Counter Experimental Hall. Booster Facility. e - e + Linac. Contents. KEKB (B-Factory) BELLE K2K at 12-GeV PS

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Water-based Antineutrino Detection

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Consequences of 3 Family oscillation:

Oscillation maximum 1.27 D m 2 L / E = p /2 Atmospheric D m 2 = 2.5 10 -3 eV 2 L = 500 km @ 1 GeV Solar D m 2 = 7 10 -5 eV 2 L = 18000km @ 1 GeV. Consequences of 3 Family oscillation:

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Status of Super-Kamiokande, K2K and JHF n

Status of Super-Kamiokande, K2K and JHF n. Yuichi Oyama (KEK). for Super-Kamiokande collaboration,. K2K collaboration and JHF n collaboration. Dec-15-2003. ACFA LC WS @Mumbai. Super-Kamiokande. 50kt water Cherenkov detector with 11146 20-inch F PMTs. ?.

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SUPER -KAMIOKANDE

SUPER -KAMIOKANDE. Kamiokande = Kamioka Nucleon Decay Experiment. Topics of Discussion. Detector Super-Kamiokande Solar neutrinos Results. Properties of Super-K. A Large Water Cherenkov Detector for Cosmic Particles Size: Cylinder of 41.4m (Height) x 39,9m (Diameter)

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JHFnu (phase I) neutrino oscillation experiment

NOON03 ? Kanazawa Feb. 11, 2003. JHFnu (phase I) neutrino oscillation experiment. For JHF-SK Neutrino Experiment collaboration Atsuko Kondo-Ichikawa KEK. Three Flavor Mixing. D m 2 12 , D m 2 23. q 12 , q 23 , q 13 + d. MNS (Maki-Nakagawa-Sakata) matrix. 3-flavor Oscillation. m 3.

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Neutrino Mass

Neutrino Mass. By Ben Heimbigner. Overview of the Presentation. History of the Neutrino Neutrino Oscillations and the relation to mass. Observations of Neutrinos Super Kamiokande (Super K) Sudbury Neutrino Observatory (SNO). What is a Neutrino?.

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JHF-Kamioka Neutrino Oscillation Experiment using JHF 50 GeV PS

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Cherenkov Tracking Calorimeters

Cherenkov Tracking Calorimeters. D. Casper University of California, Irvine. Outline. Overview Basic performance around 1 GeV Neutrino response. Acknowledgements and Caveats. Some work done together with: J. Dunmore, C. Regis (UCI)

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Neutrino Oscillations Michiel Bosma

Neutrino Oscillations Michiel Bosma. Why study neutrino oscillations ? What are neutrino oscillations ? How could one detect them ? Have neutrino oscillations been found to exist ?. Why study neutrino oscillations ?. It might partially solve the dark matter problem since:.

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