'Sk ii' diaporamas de présentation

Experimental Review of Supernova Relic Neutrinos

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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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Low Energy Challenges in SK-III

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Super-Kamiokande

Twenty Years After SN1987A, February 25, 2007. M.Nakahata. Kamioka observatory ICRR, Univ. of Tokyo. Super-Kamiokande. for SK collaboration. Super-Kamiokande detector Sensitivity of SK to supernova burst neutrinos Supernova burst search Supernova relic neutrinos Conclusions.

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data

data

290 views • 21 slides

Solar neutrino measurement at Super Kamiokande

Solar neutrino measurement at Super Kamiokande. ICHEP'04 ICRR K.Ishihara for SK collaboration. Super Kamiokande detector Result from SK-I Status of SK-II Future plan. Super Kamiokande detector. Feature of solar neutrino observation 8 B neutrino measurement by ?? + e - ? ?? + e -

363 views • 18 slides

L/E analysis of the atmospheric neutrino data from Super-Kamiokande

L/E analysis of the atmospheric neutrino data from Super-Kamiokande. Itaru Higuchi ICRR for Super-Kamiokande collaboration. ICRC2005 Aug, 2005. Motivation. Other models can explain zenith angle dependent muon deficit. How can we distinguish oscillation from other hypotheses ?

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Entry Details

117 views • 11 slides