Evidence for an oscillatory signature in atmospheric neutrino oscillations.

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; JL, Stone; LR, Sulak; CW, Walter; W, Wang; M, Goldhaber; D, Casper; JP, Cravens; W, Gajewski; WR, Kropp; DW, Liu; S, Mine; MB, Smy; HW, Sobel; CW, Sterner; MR, Vagins; KS, Ganezer; J, Hill; WE, Keig; JS, Jang; JY, Kim; IT, Lim; RW, Ellsworth; S, Tasaka; G, Guillian; A, Kibayashi; JG, Learned; S, Matsuno; D, Takemori; MD, Messier; Y, Hayato; AK, Ichikawa; T, Ishida; T, Ishii; T, Iwashita; T, Kobayashi; T, Maruyama; K, Nakamura; K, Nitta; Y, Oyama; M, Sakuda; Y, Totsuka; AT, Suzuki; M, Hasegawa; K, Hayashi; T, Inagaki; I, Kato; H, Maesaka; T, Morita; T, Nakaya; K, Nishikawa; T, Sasaki; S, Ueda; S, Yamamoto; TJ, Haines; S, Dazeley; S, Hatakeyama; R, Svoboda; E, Blaufuss; JA, Goodman; GW, Sullivan; D, Turcan; K, Scholberg; A, Habig; Y, Fukuda; CK, 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; SB, Kim; J, Yoo; H, Okazawa; T, Ishizuka; Y, Choi; HK, 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; HG, Berns; R, Gran; KK, Shiraishi; A, Stachyra; K, Washburn; RJ, Wilkes

doi:10.1103/physrevlett.93.101801

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Evidence for an oscillatory signature in atmospheric neutrino oscillations.

Shared by NobleBlocks on Sep 3, 2004 • 12:00 AM UTC

Authors:

Ashie Y

Hosaka J

Ishihara K

Abstract

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 constrai...

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