Evidence for an oscillatory signature in atmospheric neutrino oscillations.

نویسندگان

  • Y Ashie
  • J Hosaka
  • K Ishihara
  • Y Itow
  • J Kameda
  • Y Koshio
  • A Minamino
  • C Mitsuda
  • M Miura
  • S Moriyama
  • M Nakahata
  • T Namba
  • R Nambu
  • Y Obayashi
  • M Shiozawa
  • Y Suzuki
  • Y Takeuchi
  • K Taki
  • S Yamada
  • M Ishitsuka
  • T Kajita
  • K Kaneyuki
  • S Nakayama
  • A Okada
  • K Okumura
  • T Ooyabu
  • C Saji
  • Y Takenaga
  • S Desai
  • E Kearns
  • S Likhoded
  • J L Stone
  • L R Sulak
  • C W Walter
  • W Wang
  • M Goldhaber
  • D Casper
  • J P Cravens
  • W Gajewski
  • W R Kropp
  • D W Liu
  • S Mine
  • M B Smy
  • H W Sobel
  • C W Sterner
  • M R Vagins
  • K S Ganezer
  • J Hill
  • W E Keig
  • J S Jang
  • J Y Kim
  • I T Lim
  • R W Ellsworth
  • S Tasaka
  • G Guillian
  • A Kibayashi
  • J G Learned
  • S Matsuno
  • D Takemori
  • M D Messier
  • Y Hayato
  • A K Ichikawa
  • T Ishida
  • T Ishii
  • T Iwashita
  • T Kobayashi
  • T Maruyama
  • K Nakamura
  • K Nitta
  • Y Oyama
  • M Sakuda
  • Y Totsuka
  • A T Suzuki
  • M Hasegawa
  • K Hayashi
  • T Inagaki
  • I Kato
  • H Maesaka
  • T Morita
  • T Nakaya
  • K Nishikawa
  • T Sasaki
  • S Ueda
  • S Yamamoto
  • T J Haines
  • S Dazeley
  • S Hatakeyama
  • R Svoboda
  • E Blaufuss
  • J A Goodman
  • G W Sullivan
  • D Turcan
  • K Scholberg
  • A Habig
  • Y Fukuda
  • C K Jung
  • T Kato
  • K Kobayashi
  • M Malek
  • C Mauger
  • C McGrew
  • A Sarrat
  • E Sharkey
  • C Yanagisawa
  • T Toshito
  • K Miyano
  • N Tamura
  • J Ishii
  • Y Kuno
  • Y Nagashima
  • M Takita
  • M Yoshida
  • S B Kim
  • J Yoo
  • H Okazawa
  • T Ishizuka
  • Y Choi
  • H K Seo
  • Y Gando
  • T Hasegawa
  • K Inoue
  • J Shirai
  • A Suzuki
  • M Koshiba
  • Y Nakajima
  • K Nishijima
  • T Harada
  • H Ishino
  • R Nishimura
  • Y Watanabe
  • D Kielczewska
  • J Zalipska
  • H G Berns
  • R Gran
  • K K Shiraishi
  • A Stachyra
  • K Washburn
  • R J Wilkes
چکیده

Muon neutrino disappearance probability as a function of neutrino flight length L over neutrino energy E was studied. A dip in the L/E distribution was observed in the data, as predicted from the sinusoidal flavor transition probability of neutrino oscillation. The observed L/E distribution constrained nu(micro)<-->nu(tau) neutrino oscillation parameters; 1.9x10(-3)0.90 at 90% confidence level.

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عنوان ژورنال:
  • Physical review letters

دوره 93 10  شماره 

صفحات  -

تاریخ انتشار 2004