Authors
E Aliu, S Andringa, S Aoki, J Argyriades, K Asakura, R Ashie, H Berns, H Bhang, A Blondel, S Borghi, J Bouchez, J Burguet-Castell, D Casper, C Cavata, A Cervera, KO Cho, JH Choi, Ubaldo Dore, X Espinal, M Fechner, E Fernandez, Y Fukuda, J Gomez-Cadenas, R Gran, T Hara, M Hasegawa, T Hasegawa, K Hayashi, Y Hayato, RL Helmer, J Hill, K Hiraide, J Hosaka, AK Ichikawa, M Iinuma, A Ikeda, T Inagaki, T Ishida, K Ishihara, T Ishii, M Ishitsuka, Y Itow, T Iwashita, HI Jang, EJ Jeon, IS Jeong, K Joo, G Jover, CK Jung, T Kajita, J Kameda, K Kaneyuki, I Kato, E Kearns, D Kerr, CO Kim, M Khabibullin, A Khotjantsev, D Kielczewska, JY Kim, S Kim, P Kitching, K Kobayashi, T Kobayashi, A Konaka, Y Koshio, W Kropp, J Kubota, Yu Kudenko, Y Kuno, T Kutter, J Learned, S Likhoded, IT Lim, Pier Ferruccio Loverre, L Ludovici, H Maesaka, J Mallet, Camillo Mariani, T Maruyama, S Matsuno, V Matveev, C Mauger, K McConnel, C McGrew, S Mikheyev, A Minamino, S Mine, O Mineev, C Mitsuda, M Miura, Y Moriguchi, T Morita, S Moriyama, T Nakadaira, M Nakahata, K Nakamura, I Nakano, T Nakaya, S Nakayama, T Namba, R Nambu, S Nawang, K Nishikawa, K Nitta, Federico Nova, P Novella, Y Obayashi, A Okada, K Okumura, SM Oser, Y Oyama, MY Pac, F Pierre, A Rodriguez, C Saji, M Sakuda, F Sanchez, A Sarrat, T Sasaki, K Scholberg, R Schroeter, M Sekiguchi, E Sharkey, M Shiozawa, K Shiraishi, G Sitjes, M Smy, H Sobel, J Stone, L Sulak, A Suzuki, Y Suzuki, T Takahashi, Y Takenaga, Y Takeuchi, K Taki, Y Takubo, N Tamura, M Tanaka, R Terri, S T'jampens, A Tornero-Lopez, Y Totsuka, S Ueda, M Vagins, CW Walter, W Wang, RJ Wilkes, S Yamada
Publication date
2005/3/4
Journal
Physical Review Letters
Volume
94
Issue
8
Pages
081802
Publisher
American Physical Society
Description
We present results for oscillation in the KEK to Kamioka (K2K) long-baseline neutrino oscillation experiment. K2K uses an accelerator-produced beam with a mean energy of 1.3 GeV directed at the Super-Kamiokande detector. We observed the energy-dependent disappearance of , which we presume have oscillated to . The probability that we would observe these results if there is no neutrino oscillation is 0.0050% ().
Total citations
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Scholar articles
E Aliu, S Andringa, S Aoki, J Argyriades, K Asakura… - Physical Review Letters, 2005