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KAMIOKA nucleon decay experiment
Authors:M. Koshiba
Affiliation:(1) ICEPP, Faculty of Science, University of Tokyo, Tokyo, Japan
Abstract:Summary Recent results of KAMIOKA nucleon decay experiment are presented. The great majority, ∼95%, of the contained events can be naturally explained as due to the atmospheric neutrinos,i.e. the rate and the momentum distribution of the pseudoelastic νμ and νe events and the multiplicity distribution. However, 5 multiple-ring events remain each defying this interpretation at 90% c.l. Stringent flux upper limits are obtained for magnetic monopole from the searches for Rubakov effect in the detector and in the Sun. KAMIOKANDE collaboration:K. Arisaka, T. Kajita, T. Kifune, M. Koshiba, K. Miyano, M. Nakahata, Y. Oyama, T. Suda, A. Suzuki, K. Takahashi, M. Takita andY. Totsuka: ICEPP and Department of Physics, University of Tokyo; Institute of Cosmic Ray Research, University of Tokyo; KEK, National Laboratory for High Energy Physics and Department of Physics, Niigata University. (As of January 1985,K. Arisaka moved to Department of Physics, Pennsilvania University.)
Keywords:Cosmic rays
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