Phys. Rev. Lett.
81,
2016–2019
(1998)
Measurement of the Flux and Zenith-Angle Distribution of Upward Through-Going Muons in Kamiokande II+III
S. Hatakeyama et al.
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S. Hatakeyama1, T. Hara2, Y. Fukuda3, T. Hayakawa3, K. Inoue3, K. Ishihara3, H. Ishino3, S. Joukou3, T. Kajita3, S. Kasuga3, Y. Koshio3, T. Kumita3,*, K. Matsumoto3, M. Nakahata3, K. Nakamura3,†, K. Okumura3, A. Sakai3,‡, M. Shiozawa3, J. Suzuki3, Y. Suzuki3, T. Tomoeda3, Y. Totsuka3, K. S. Hirata4, K. Kihara4, Y. Oyama4,§, M. Koshiba5,**, K. Nishijima6, T. Horiuchi6, K. Fujita1, M. Koga1, T. Maruyama1, A. Suzuki1, M. Mori7,††, T. Suda8,‡‡, A. T. Suzuki8, T. Ishizuka9, K. Miyano9, H. Okazawa9, Y. Nagashima2, M. Takita2, T. Yamaguchi2, Y. Hayato10,a, K. Kaneyuki10, T. Suzuki10, Y. Takeuchi10,b, T. Tanimori10, S. Tasaka11, E. Ichihara12, S. Miyamoto12, and K. Nishikawa12,c
1Physics Department, Graduate School of Science, Tohoku University, Sendai, Miyagi 980-8578, Japan 2High Energy Physics Division, Graduate School of Science, Osaka University, Toyonaka, Osaka 560-0043, Japan 3Institute for Cosmic Ray Research, University of Tokyo, Tanashi, Tokyo 188-8502, Japan 4National Laboratory for High Energy Physics, Tsukuba, Ibaraki 305-0801, Japan 5Institute of Research and Development, Tokai University, Shibuya, Tokyo 151-0063, Japan 6Department of Physics, Tokai University, Hiratsuka, Kanagawa 259-1292, Japan 7Department of Physics, Miyagi University of Education, Sendai, Miyagi 980-0845, Japan 8Department of Physics, Kobe University, Kobe, Hyogo 657-8501, Japan 9Niigata University, Niigata 950-2181, Japan 10Department of Physics, Tokyo Institute of Technology, Megro-ku, Tokyo 152-8551, Japan 11Department of Physics, Gifu University, Gifu, Gifu 501-1193, Japan 12Institute for Nuclear Study, University of Tokyo, Tanashi, Tokyo 188-8501, Japan
Received 2 June 1998; published in the issue dated 7 September 1998
The flux of upward through-going muons of minimum (mean) threshold energy >1.6 (3.0) GeV is measured, based on a total of 372 events observed by the Kamiokande II+III detector during 2456 detector live days. The observed muon flux was Φobs = [1.94±0.10(stat.)-0.06+0.07sys.)]×10-13cm-2s-1sr-1, which is compared to an expected value of Φtheo = [2.46±0.54(theo.)]×10-13cm-2s-1sr-1. The observation is in agreement with the prediction within the errors. The zenith-angle dependence of the observed upward through-going muons supports the previous indication of neutrino oscillations made by Kamiokande using sub- and multi-GeV atmospheric neutrino events.
© 1998 The American Physical Society
URL:
http://link.aps.org/doi/10.1103/PhysRevLett.81.2016
DOI:
10.1103/PhysRevLett.81.2016
*Present address: Department of Physics, Tokyo Metropolitan University, Hachiouji, Tokyo 192-0397, Japan. †Present address: High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan. ‡ § **Present address: The University of Tokyo, Tokyo 113-0033, Japan. ††Present address: Institute for Cosmic Ray Research, University of Tokyo, Tanashi, Tokyo 188-8502, Japan. ‡‡Deceased. a b c
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