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Measurement of atmospheric neutrino oscillation parameters by Super-Kamiokande I

Authors :
G. Guillian
C. Yanagisawa
M. Goldhaber
A. K. Ichikawa
K. Kaneyuki
A. Minamino
Y. Watanabe
S. Mine
D. W. Liu
Atsumu Suzuki
S. Matsuno
E. Kearns
T. Toshito
Hirokazu Ishino
M. Ishitsuka
Y. Totsuka
A. Suzuki
C. W. Walter
Ko Okumura
R. Svoboda
D. Turcan
Shantanu Desai
Y. Nakajima
K. Ishihara
J. P. Cravens
Y. Ashie
C. McGrew
S. Clark
R. J. Wilkes
Tsuyoshi Nakaya
Kunio Inoue
Y. Hayato
K. Taki
T. Sasaki
C. Saji
J. Yoo
A. L. Stachyra
K. Nishikawa
I. T. Lim
Masato Shiozawa
A. Kibayashi
K. S. Ganezer
J. Kameda
Shoji Yamamoto
T. Kato
N. Tamura
L. R. Sulak
C. W. Sterner
E. Blaufuss
J. Shirai
Y. Fukuda
Magdalena Malek
J. L. Stone
E. Sharkey
S. Dazeley
Yoshitaka Itow
Takashi Kobayashi
K. Hayashi
Y. Gando
Yusuke Koshio
Koji Nakamura
Y. Takeuchi
K. Washburn
Mark R. Vagins
John G. Learned
T. Iwashita
H. Okazawa
S. Ueda
T. Maruyama
S. Likhoded
Shinya Yamada
R. Nambu
W. Wang
S. Hatakeyama
Y. Kuno
R. Gran
Kazumasa Miyano
Henry W. Sobel
K. Nitta
Michael B. Smy
H. Seo
Takehisa Hasegawa
Kyoshi Nishijima
J. A. Goodman
Alec Habig
W. R. Kropp
G. W. Sullivan
John Hill
C. K. Jung
D. Kielczewska
Shigetaka Moriyama
J. S. Jang
D. Takemori
Yuichi Oyama
I. Kato
Shoei Nakayama
Katsuhiro Kobayashi
Minoru Yoshida
Y. Obayashi
T. Harada
S. Tasaka
W. E. Keig
T. Ishii
W. Gajewski
Kate Scholberg
S. B. Kim
David William Casper
Masayuki Nakahata
C. Mitsuda
J. Hosaka
Y. Takenaga
Masaya Hasegawa
M. Miura
K. K. Shiraishi
Yoshihiro Suzuki
Masatoshi Koshiba
J. Ishii
J. Zalipska
T. Ishida
Makoto Sakuda
A. Sarrat
Todd Haines
M. D. Messier
C. Mauger
A. Okada
H. G. Berns
T. Ishizuka
Taichi Morita
R. W. Ellsworth
Takaaki Kajita
Y. Choi
J. Y. Kim
Toshio Namba
H. Maesaka
Source :
Physical Review D. 71
Publication Year :
2005
Publisher :
American Physical Society (APS), 2005.

Abstract

We present a combined analysis of fully-contained, partially-contained and upward-going muon atmospheric neutrino data from a 1489 day exposure of the Super--Kamiokande detector. The data samples span roughly five decades in neutrino energy, from 100 MeV to 10 TeV. A detailed Monte Carlo comparison is described and presented. The data is fit to the Monte Carlo expectation, and is found to be consistent with neutrino oscillations of $\nu_\mu \leftrightarrow \nu_\tau$ with $\sin^22\theta > 0.92$ and $1.5\times 10^{-3} < \Delta m^2 < 3.4\times 10^{-3}{\rm eV}^2$ at 90% confidence level.<br />Comment: 32 pages, 44 figures. As accepted for publication in Physical Review D

Details

ISSN :
15502368 and 15507998
Volume :
71
Database :
OpenAIRE
Journal :
Physical Review D
Accession number :
edsair.doi.dedup.....a36b2c4676a964a766a5f0db4fb1bba4