Abstract
The initial concept of Kamiokande was proposed by Koshiba in 1979. This idea was presented by one of his collaborators at a workshop on the unified theory and the baryon number in the universe [1]. The detector considered is shown in Fig.l. It comprises water Čerenkov counters A and B, and is located deep underground. Counter B is used to detect nucléon decay which occurs in water within the detector. To be specific, the size is 20 × 20 × 5 m3, containing 2000 tons of water. The surface is covered with 7500 5-inch photomultiplier tubes (PMT’s), one in every 40 × 40 cm2. The inside of the box is painted black so as to avoid any reflection of the Čerenkov light: the direction and, in some cases, energy of charged particles and γ-rays can then be measured. Counter A has a size of 25 × 25 × 0.1 m3, and is placed above counter B while serving as an anticounter to veto atmospheric muons that penetrate. The inside of this counter is painted white, and the water is dissolved with a wavelength shifter so as to increase the light yield, which reduces the number of necessary phototubes: one hundred tubes are hopefully more than enough. These are pasted onto the top surface of the counter. A steel plate having a thickness 25 cm between counters A and B is used to stop any charged particles produced by nucléon decays in counter B. Fig. 2 illustrates how the p → μ+ + γ decay mode would be detected in this detector.
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Suzuki, A. (1994). Kamiokande: Historical Account. In: Fukugita, M., Suzuki, A. (eds) Physics and Astrophysics of Neutrinos. Springer, Tokyo. https://doi.org/10.1007/978-4-431-67029-2_3
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DOI: https://doi.org/10.1007/978-4-431-67029-2_3
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