Publications [#248871] of Christopher Walter

Papers Published
  1. Ashie, Y; Hosaka, J; Ishihara, K; Itow, Y; Kameda, J; Koshio, Y; Minamino, A; Mitsuda, C; Miura, M; Moriyama, S; Nakahata, M; Namba, T; Nambu, R; Obayashi, Y; Shiozawa, M; Suzuki, Y; Takeuchi, Y; Taki, K; Yamada, S; Ishitsuka, M; Kajita, T; Kaneyuki, K; Nakayama, S; Okada, A; Okumura, K; Ooyabu, T; Saji, C; Takenaga, Y; Desai, S; Kearns, E; Likhoded, S; Stone, JL; Sulak, LR; Walter, CW; Wang, W; Goldhaber, M; Casper, D; Cravens, JP; Gajewski, W; Kropp, WR; Liu, DW; Mine, S; Smy, MB; Sobel, HW; Sterner, CW; Vagins, MR; Ganezer, KS; Hill, J; Keig, WE; Jang, JS; Kim, JY; Lim, IT; Ellsworth, RW; Tasaka, S; Guillian, G; Kibayashi, A; Learned, JG; Matsuno, S; Takemori, D; Messier, MD; Hayato, Y; Ichikawa, AK; Ishida, T; Ishii, T; Iwashita, T; Kobayashi, T; Maruyama, T; Nakamura, K; Nitta, K; Oyama, Y; Sakuda, M; Totsuka, Y; Suzuki, AT; Hasegawa, M; Hayashi, K; Inagaki, T; Kato, I; Maesaka, H; Morita, T; Nakaya, T; Nishikawa, K; Sasaki, T; Ueda, S; Yamamoto, S; Haines, TJ; Dazeley, S; Hatakeyama, S; Svoboda, R; Blaufuss, E; Goodman, JA; Sullivan, GW; Turcan, D; Scholberg, K; Habig, A; Fukuda, Y; Jung, CK; Kato, T; Kobayashi, K; Malek, M; Mauger, C; McGrew, C; Sarrat, A; Sharkey, E; Yanagisawa, C; Toshito, T; Miyano, K; Tamura, N; Ishii, J; Kuno, Y; Nagashima, Y; Takita, M; Yoshida, M; Kim, SB; Yoo, J; Okazawa, H; Ishizuka, T; Choi, Y; Seo, HK; Gando, Y; Hasegawa, T; Inoue, K; Shirai, J; Suzuki, A; Koshiba, M; Nakajima, Y; Nishijima, K; Harada, T; Ishino, H; Nishimura, R; Watanabe, Y; Kielczewska, D; Zalipska, J; Berns, HG; Gran, R; Shiraishi, KK; Stachyra, A; Washburn, K; Wilkes, RJ; Super-Kamiokande Collaboration,, Evidence for an oscillatory signature in atmospheric neutrino oscillations., Physical Review Letters, vol. 93 no. 10 (September, 2004), pp. 101801 [15447395], [doi] .

    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 constrained nu(micro)<-->nu(tau) neutrino oscillation parameters; 1.9x10(-3)0.90 at 90% confidence level.