Super-Kamiokande

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Atmospheric Neutrinos Summary Oscillation analysis result based on SK-1 (1489d) +SK- 2(890d) is presented Further analysis based on SK-I(1489d) Consistent with nm nt oscillation. Some non-tau modes: unlikely Solar Neutrinos Oscillation analysis based on SK-I(1469d) is presented SK-II data also analyzed though energy threshold is 7MeV Improvements for SK-III is going on Upper limits for SN and SRN rate obtained May 26, 2006 Y.Obayashi @ Vulcano 2006 30
Supplements May 26, 2006 Y.Obayashi @ Vulcano 2006 31
Page 1 and 2: May 26, 2006 Vulcano Workshop 2006
Page 3 and 4: 42 m Super-Kamiokande • 50kton pu
Page 5 and 6: Overview Atmospheric Neutrinos nm d
Page 7 and 8: May 26, 2006 Y.Obayashi @ Vulcano 2
Page 9 and 10: L/E analysis Update from Phys. Rev.
Page 13 and 14: Tau Appearance Search • Tau Enric
Page 17 and 18: Solar n Data of SK-I May 31, 1996 -
Page 25 and 26: P(n e → n e ) E May 26, 2006 n (M
Page 27 and 28: Improvement May 26, 2006 Y.Obayashi
Page 29: May 26, 2006 Y.Obayashi @ Vulcano 2
Page 35 and 36: SK-I + SK-II combined analysis (dat
Page 37 and 38: Result from SK-I + SK-II data SK-I

Super-Kamiokande

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