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Measurement of the Flux and Zenith-Angle Distribution of Upward Throughgoing Muons by Super-Kamiokande

Authors :
L. R. Price
J. Shirai
E. Sharkey
C. K. Jung
S. Mine
M. Takahata
D. Kielczewska
J. W. Flanagan
Y. Kanaya
Hiroshi Ogawa
Takehisa Hasegawa
Y. Hayato
Y. Watanabe
R. Sanford
J. A. Goodman
Kazumasa Miyano
Minoru Yoshida
H. Okazawa
T. Iwamoto
Ken-ichiro Kobayashi
David William Casper
E. Ichihara
C. W. Walter
Yuichi Oyama
F. Tsushima
Todd Haines
W. Doki
S. Hatakeyama
Takaaki Kajita
H. Ishino
A. Sakai
Yusuke Koshio
L. Wai
Michael B. Smy
Nobuyuki Sakurai
W. E. Keig
Mark R. Vagins
Tomoyuki Maruyama
T. Kobayashi
C. Mauger
Makoto Sakuda
Junichi Kanzaki
K. Nakamura
J. Kameda
B. Viren
M. Miura
Frederick Reines
Ko Okumura
Masatoshi Koshiba
T. Hayakawa
S. Matsuno
T. Ishii
M. D. Messier
Soo-Bong Kim
S. Kasuga
Y. Fukuda
M. Goldhaber
S. Echigo
Yasunari Suzuki
K. Martens
V. J. Stenger
A. Suzuki
R. Svoboda
A. Okada
S. Tasaka
W. R. Kropp
Atsumu Suzuki
A. Kibayashi
Masayuki Nakahata
Y. Totsuka
J. L. Stone
C. Yanagisawa
K. Fujita
E. Kearns
M. L. Chen
W. Gajewski
Kate Scholberg
Kunio Inoue
C. McGrew
K. Ishihara
M. Takita
Y. Takeuchi
K. Kaneyuki
C. Saji
M. Earl
E. Blaufuss
Shinya Yamada
M. Etoh
Masato Shiozawa
K. S. Ganezer
A. L. Stachyra
John G. Learned
Yoshitaka Itow
T. Barszczak
Kyoshi Nishijima
Takashi Yamaguchi
R. W. Ellsworth
R. A. Doyle
T. Futagami
R. J. Wilkes
K. K. Young
Y. Kobayashi
G. W. Sullivan
M. Kohama
Alec Habig
J. S. George
M. Nemoto
L. R. Sulak
M. Koga
H. W. Sobel
Osamu Sasaki
D. Takemori
Shoei Nakayama
K. Nishikawa
J. Hill
Y. Nagashima
B. K. Kim
Akira Hasegawa
Source :
Physical Review Letters. 82:2644-2648
Publication Year :
1999
Publisher :
American Physical Society (APS), 1999.

Abstract

A total of 614 upward through-going muons of minimum energy 1.6 GeV are observed by Super-Kamiokande during 537 detector live days. The measured muon flux is 1.74+/-0.07(stat.)+/-0.02(sys.)x10^{-13}cm^{-2}s^{-1}sr^{-1} compared to an expected flux of 1.97+/-0.44(theo.)x10^{-13}cm^{-2}s^{-1}sr^{-1}. The absolute measured flux is in agreement with the prediction within the errors. However, the zenith angle dependence of the observed upward through-going muon flux does not agree with no-oscillation predictions. The observed distortion in shape is consistent with the \nu_\mu \nu_\tau oscillation hypothesis with \sin^22\theta > 0.4 and 1x10^{-3} < \Delta m^2 < 1x10^{-1} eV^{2} at 90% confidence level.<br />Comment: 8 pages w/ 3 figures new version contains minor fixes, as it appears in PRL

Details

ISSN :
10797114 and 00319007
Volume :
82
Database :
OpenAIRE
Journal :
Physical Review Letters
Accession number :
edsair.doi.dedup.....c14a9743da04de7eb034a2dcbf9e3d4e
Full Text :
https://doi.org/10.1103/physrevlett.82.2644