Abstract
The recent results of the atmospheric neutrino measurements and neutrino oscillation analysis from Super-Kamiokande are presented. The Super-Kamiokande detector is observing the atmospheric neutrinos in the wide energy range from 0.1 GeV to 10 TeV. The data are fully consistent with two flavor νµ ↔ ντ oscillation scheme. We slightly improved the oscillation analysis method, which gives more stringent constraint on the oscillation parameters. The searches are made for the tau neutrino signal from νµ ↔ ντ oscillation and the effect of non-zero θ13 mixing angle. The preliminary result of Super-Kamiokande II data will be also mentioned.
Similar content being viewed by others
References
M. Nakahata et al. (Super-Kamiokande) Nucl. Instrum. Meth A501, 418 (2003)
Y. Ashie et al. (Super-Kamiokande), Phys. Rev. D71, 112005 (2005)
Y. Ashie et al. (Super-Kamiokande), Phys. Rev. Lett. 93, 101801 (2004)
M. Apollonio et al. (CHOOZ), Phys. Lett. B466, 415 (1999)
E. Aliu et al. (K2K) Phys. Rev. Lett. 94, 081802 (2005)
S. P. Mikheyev and A. Y. Smirnov, Yad. Fiz. 42, 1441 (1985)
S. P. Mikheyev and A. Y. Smirnov, Nuov. Cim. C9, 17 (1986)
L. Wolfenstein, Phys. Rev. D20, 2634 (1979)
Author information
Authors and Affiliations
Additional information
For The Super-Kamiokande collaboration
Rights and permissions
About this article
Cite this article
Okumura, K. Super-Kamiokande atmospheric neutrino results. Czech J Phys 56 (Suppl 1), A271–A280 (2006). https://doi.org/10.1007/s10582-006-0161-z
Received:
Issue Date:
DOI: https://doi.org/10.1007/s10582-006-0161-z