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A Measurement of Atmospheric Neutrino Flux Consistent with Tau Neutrino Appearance

Authors :
K. Kaneyuki
W. R. Kropp
R. J. Wilkes
Y. Takeuchi
Yasunari Suzuki
G. Mitsuka
I. T. Lim
T. Iwashita
Takaaki Kajita
I. Higuchi
Henry W. Sobel
K. Nitta
T. Nakadaira
Kyoshi Nishijima
A. K. Ichikawa
Michael Litos
Frédéric Dufour
M. Ishitsuka
S. B. Kim
J. Y. Kim
Atsushi Takeda
J. Kameda
Makoto Sakuda
A. Minamino
Shigetaka Moriyama
H. Ishii
Atsumu Suzuki
Shantanu Desai
Minoru Yoshida
K. Nakamura
N. Tamura
C. Regis
M. Sugihara
Y. Totsuka
C. K. Jung
Shoei Nakayama
Yuichi Oyama
J. L. Stone
D. Kielczewska
E. Kearns
T. Ishii
D. W. Liu
M. Malek
Y. Gando
C. McGrew
S. Clark
J. P. Cravens
K. Ishihara
J. Hill
K. S. Ganezer
Yusuke Koshio
I. Kato
Masayuki Nakahata
Y. Watanabe
C. Yanagisawa
H. Okazawa
Y. Takenaga
Mark R. Vagins
Masaya Hasegawa
M. Miura
C. W. Walter
J. S. Jang
K. Abe
L. R. Sulak
C. Saji
J. Zalipska
K. Nishikawa
T. Iida
Y. Obayashi
K. Ueshima
T. Sato
J. Yoo
E. Guillian
T. Ishida
Masato Shiozawa
Y. Choi
M. Goldhaber
David William Casper
R. A. Wendell
C. Mitsuda
H. Ogawa
S. Mine
W. Wang
J. G. Learned
Todd Haines
T. Koike
Kate Scholberg
Yoshitaka Itow
G. W. Sullivan
M. D. Messier
T. Kobayashi
K. K. Shiraishi
Y. Fukuda
C. Ishihara
K. Washburn
Katsuhiro Kobayashi
T. Ishizuka
Masashi Yokoyama
R. Svoboda
S. Hatakeyama
R. Gran
J. L. Raaf
Ko Okumura
H. G. Berns
R. W. Ellsworth
Tsuyoshi Nakaya
Takehisa Hasegawa
Hirokazu Ishino
R. Terri
Masatoshi Koshiba
Kunio Inoue
S. Likhoded
Y. Kuno
Takanori Sasaki
T. Kato
A. Sarrat
Michael B. Smy
H. Seo
W. E. Keig
N. Tanimoto
H. Maesaka
Hiroshi Sato
H. Nishino
Shigeki Tasaka
S. Dazeley
Y. Hayato
Alec Habig
S. Matsuno
Shoji Yamamoto
Publication Year :
2006

Abstract

A search for the appearance of tau neutrinos from \mutau oscillations in the atmospheric neutrinos has been performed using 1489.2 days of atmospheric neutrino data from the Super-Kamiokande-I experiment. A best fit tau neutrino appearance signal of 138 $\pm$ 48 (stat.) $^{+15}_{-32}$ (sys.) events is obtained with an expectation of 78 $\pm$ 26 (sys.). The hypothesis of no tau neutrino appearance is disfavored by 2.4 sigma.<br />Comment: 5 pages, 3 figures, 3 tables, submitted to PRL

Details

Language :
English
Database :
OpenAIRE
Accession number :
edsair.doi.dedup.....5e999bb8b3ff20336f5d48c6be9620b9