- Main
Atmospheric neutrino oscillation analysis with improved event reconstruction in Super-Kamiokande IV
- Jiang, M;
- Abe, K;
- Bronner, C;
- Hayato, Y;
- Ikeda, M;
- Iyogi, K;
- Kameda, J;
- Kato, Y;
- Kishimoto, Y;
- Marti, LL;
- Miura, M;
- Moriyama, S;
- Mochizuki, T;
- Nakahata, M;
- Nakajima, Y;
- Nakano, Y;
- Nakayama, S;
- Okada, T;
- Okamoto, K;
- Orii, A;
- Pronost, G;
- Sekiya, H;
- Shiozawa, M;
- Sonoda, Y;
- Takeda, A;
- Takenaka, A;
- Tanaka, H;
- Yano, T;
- Akutsu, R;
- Kajita, T;
- Nishimura, Y;
- Okumura, K;
- Wang, R;
- Xia, J;
- Labarga, L;
- Fernandez, P;
- Blaszczyk, FDM;
- Kachulis, C;
- Kearns, E;
- Raaf, JL;
- Stone, JL;
- Sussman, S;
- Berkman, S;
- Bian, J;
- Griskevich, NJ;
- Kropp, WR;
- Locke, S;
- Mine, S;
- Weatherly, P;
- Smy, MB;
- Sobel, HW;
- Takhistov, V;
- Ganezer, KS;
- Hill, J;
- Kim, JY;
- Lim, IT;
- Park, RG;
- Bodur, B;
- Scholberg, K;
- Walter, CW;
- Gonin, M;
- Imber, J;
- Mueller, Th A;
- Ishizuka, T;
- Nakamura, T;
- Jang, JS;
- Choi, K;
- Learned, JG;
- Matsuno, S;
- Litchfield, RP;
- Uchida, Y;
- Wascko, MO;
- Calabria, NF;
- Catanesi, MG;
- Intonti, RA;
- Radicioni, E;
- De Rosa, G;
- Ali, A;
- Collazuol, G;
- Iacob, F;
- Ludovici, L;
- Cao, S;
- Friend, M;
- Hasegawa, T;
- Ishida, T;
- Kobayashi, T;
- Nakadaira, T;
- Nakamura, K;
- Oyama, Y;
- Sakashita, K;
- Sekiguchi, T;
- Tsukamoto, T;
- Abe, KE;
- Hasegawa, M;
- Isobe, Y;
- Miyabe, H;
- Sugimoto, T;
- Suzuki, AT;
- Takeuchi, Y;
- Ashida, Y;
- Hayashino, T;
- Hirota, S;
- Kikawa, T;
- Mori, M;
- Nakamura, KE;
- Nakaya, T;
- Wendell, RA;
- Anthony, LHV;
- McCauley, N;
- Pritchard, A;
- Tsui, KM;
- Fukuda, Y;
- Itow, Y;
- Murrase, M;
- Mijakowski, P;
- Frankiewicz, K;
- Jung, CK;
- Li, X;
- Palomino, JL;
- Santucci, G;
- Vilela, C;
- Wilking, MJ;
- Yanagisawa, C;
- Fukuda, D;
- Hagiwara, K;
- Ishino, H;
- Ito, S;
- Koshio, Y;
- Sakuda, M;
- Takahira, Y;
- Xu, C;
- Kuno, Y;
- Simpson, C;
- Wark, D;
- Di Lodovico, F;
- Richards, B;
- Sedgwick, S Molina;
- Tacik, R;
- Kim, SB;
- Thiesse, M;
- Thompson, L;
- Okazawa, H;
- Choi, Y;
- Nishijima, K;
- Koshiba, M;
- Yokoyama, M;
- Goldsack, A;
- Martens, K;
- Murdoch, M;
- Quilain, B;
- Suzuki, Y;
- Vagins, MR;
- Kuze, M;
- Okajima, Y;
- Yoshida, T;
- Ishitsuka, M;
- Martin, JF;
- Nantais, CM;
- Tanaka, HA;
- Towstego, T;
- Hartz, M;
- Konaka, A;
- de Perio, P;
- Chen, S;
- Wan, L;
- Minamino, A
- et al.
Abstract
A new event reconstruction algorithm based on a maximum likelihood method has been developed for Super-Kamiokande. Its improved kinematic and particle identification capabilities enable the analysis of atmospheric neutrino data in a detector volume 32% larger than previous analyses and increase the sensitivity to the neutrino mass hierarchy.Analysis of a 253.9 kton•year exposure of the Super-Kamiokande IV atmospheric neutrino data has yielded a weak preference for the normal hierarchy, disfavoring the inverted hierarchy at 74% assuming oscillations at the best fit of the analysis.
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