Super-Kamiokande

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May 26, 2006 Y.Obayashi @ Vulcano 2006 28 <strong>Super</strong>nova Neutrino Bursts No candidate was found in SK-I and SK-II 2.3 T < 0.39 SN/yr (90%CL) Upper limit of galactic SN rate < Efficiency vs. Distance T: measurement time
May 26, 2006 Y.Obayashi @ Vulcano 2006 29 <strong>Super</strong>novae Relic Neutrinos Reactor n Solar 8 B Solar hep Expectations Population synthesis (Totani et al., 1996) Constant SN rate (Totani et al., 1996) Cosmic gas infall (Malaney, 1997) Cosmic chemical evolution (Hartmann et al., 1997) Heavy metal abundance (Kaplinghat et al., 2000) LMA n oscillation (Ando et al., 2002) Atmospheric n Phys. Rev. Lett. 90, 061101(2003) SK-I Total background Atmospheric n m → invisible m → decay e 90% CL limit of SRN Atmospheric n e
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: Improvement May 26, 2006 Y.Obayashi
Page 31 and 32: Supplements May 26, 2006 Y.Obayashi
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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