2018•Physical review. D/Physical review. D.Open access

Atmospheric neutrino oscillation analysis with external constraints in Super-Kamiokande I-IV

K. Abe, Christophe Bronner, Yuto Haga, Y. Hayato, M. Ikeda, K. Iyogi, J. Kameda, Y. Kato, Yasuaki Kishimoto, Ll. Marti, M. Miura, S. Moriyama, Masayuki Nakahata, T. Nakajima, Y. Nakano, S. Nakayama, Y. Okajima, A. Orii, G. Pronost, H. Sekiya, Masato Shiozawa, Y. Sonoda, A. Takeda, A. Takenaka, H. Tanaka, S. Tasaka, T. Tomura, R. Akutsu, T. J. Irvine, T. Kajita, Isao Kametani, K. Kaneyuki, Y. Nishimura, K. Okumura, Euan Richard, K. M. Tsui, Luis Labarga, Pablo Fernández, F. d. M. Blaszczyk, J. Gustafson, C. Kachulis, E. Kearns, Jennifer L. Raaf, J. L. Stone, L. R. Sulak, S. Berkman, S. Tobayama, M. Goldhaber, Giada Carminati, M. Elnimr, William R. Kropp, S. Mine, Scott Locke, A. Renshaw, M. B. SMY, Henry W. Sobel, Volodymyr Takhistov, P. Weatherly, K. S. Ganezer, B. L. Hartfiel, J. Hill, N. Hong, J. Y. Kim, I. T. Lim, R. G. Park, T. Akiri, A. Himmel, Zepeng Li, Erin O’Sullivan, K. Scholberg, C. W. Walter, T. Wongjirad, Tatsumi Ishizuka, T. Nakamura, J. S. Jang, Koun Choi, JOHN G. LEARNED, Shigenobu Matsuno, Stefanie N. Smith, J. L. Amey, R. P. Litchfield, Wing Yan Ma, Y. Uchida, Morgan O. Wascko, S. Cao, M. Friend, T. Hasegawa, T. Ishida, T. Ishii, T. Kobayashi, Takeshi Nakadaira, Keigo Nakamura, Y. Oyama, Ken Sakashita, Tetsuro Sekiguchi, Toshifumi Tsukamoto, KE. Abe, M. Hasegawa, Y. Suzuki, Y. Takeuchi, T. Yano, Tatsuya HAYASHINO, S. Hirota, K. Huang, K. Ieki, M. Jiang, Tatsuya Kikawa, KE. Nakamura, T. Nakaya, N. D. Patel, Ken Suzuki, Sentaro Takahashi, R. A. Wendell, Lauren H.V. Anthony, N. McCauley, A. Pritchard, Y. Fukuda, Y. Itow, G. Mitsuka, M. Murase, F. Muto, T. Suzuki, P. Mijakowski, K. Frankiewicz, J. Hignight, J. Imber, Chang Kee Jung, X. Li, J. L. Palomino, G. Santucci, C. Vilela, M. J. Wilking, C. Yanagisawa, S. Ito, D. Fukuda, H. Ishino, T. Kayano, A. Kibayashi, Y. Koshio, T. Mori, Hiroshi Nagata, M. Sakuda, Chenyuan Xu, Yoshitaka Kuno, Dave Wark, Francesca Di Lodovico, B. Richards, R. Tacik, S. B. Kim, A. Cole, Lee F. Thompson, H. Okazawa, Y. Choi, Kei Ito, K. Nishijima, Masatoshi Koshiba, Yoji Totsuka, Yusuke Suda, M. Yokoyama, R. G. Calland, M. Hartz, K. Martens, Benjamin Quilain, Charles H. Simpson, Y. Suzuki, Mark R. Vagins, D. Hamabe, M. Kuze, T. Yoshida, M. Ishitsuka, J. F. Martin, C. Nantais, Patrick de Perio, H. A. Tanaka, A. Konaka, S. Chen, L. Wan, Y. Zhang, R. Jeffrey Wilkes, A. Minamino

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Abstract

An analysis of atmospheric neutrino data from all four run periods of Super-Kamiokande optimized for sensitivity to the neutrino mass hierarchy is presented. Confidence intervals for $\mathrm{\ensuremath{\Delta}}{m}_{32}^{2}$, ${\mathrm{sin}}^{2}{\ensuremath{\theta}}_{23}$, ${\mathrm{sin}}^{2}{\ensuremath{\theta}}_{13}$ and ${\ensuremath{\delta}}_{CP}$ are presented for normal neutrino mass hierarchy and inverted neutrino mass hierarchy hypotheses, based on atmospheric neutrino data alone. Additional constraints from reactor data on ${\ensuremath{\theta}}_{13}$ and from published binned T2K data on muon neutrino disappearance and electron neutrino appearance are added to the atmospheric neutrino fit to give enhanced constraints on the above parameters. Over the range of parameters allowed at 90% confidence level, the normal mass hierarchy is favored by between 91.9% and 94.5% based on the combined Super-Kamiokande plus T2K result.

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An analysis of atmospheric neutrino data from all four run periods of Super-Kamiokande optimized for sensitivity to the neutrino mass hierarchy is presented. Confidence intervals for $\mathrm{\ensuremath{\Delta}}{m}_{32}^{2}$, ${\mathrm{sin}}^{2}{\ensuremath{\theta}}_{23}$, ${\mathrm{sin}}^{2}{\ensuremath{\theta}}_{13}$ and ${\ensuremath{\delta}}_{CP}$ are presented for normal neutrino mass hierarchy and inverted neutrino mass hierarchy hypotheses, based on atmospheric neutrino data alone. Additional constraints from reactor data on ${\ensuremath{\theta}}_{13}$ and from published binned T2K data on muon neutrino disappearance and electron neutrino appearance are added to the atmospheric neutrino fit to give enhanced constraints on the above parameters. Over the range of parameters allowed at 90% confidence level, the normal mass hierarchy is favored by between 91.9% and 94.5% based on the combined Super-Kamiokande plus T2K result.

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Available abstract

An analysis of atmospheric neutrino data from all four run periods of Super-Kamiokande optimized for sensitivity to the neutrino mass hierarchy is presented. Confidence intervals for $\mathrm{\ensuremath{\Delta}}{m}_{32}^{2}$, ${\mathrm{sin}}^{2}{\ensuremath{\theta}}_{23}$, ${\mathrm{sin}}^{2}{\ensuremath{\theta}}_{13}$ and ${\ensuremath{\delta}}_{CP}$ are presented for normal neutrino mass hierarchy and inverted neutrino mass hierarchy hypotheses, based on atmospheric neutrino data alone. Additional constraints from reactor data on ${\ensuremath{\theta}}_{13}$ and from published binned T2K data on muon neutrino disappearance and electron neutrino appearance are added to the atmospheric neutrino fit to give enhanced constraints on the above parameters. Over the range of parameters allowed at 90% confidence level, the normal mass hierarchy is favored by between 91.9% and 94.5% based on the combined Super-Kamiokande plus T2K result.

Key concepts: Neutrino, Neutrino oscillation, Physics, Particle physics, Muon, Electron neutrino, Solar neutrino problem, Solar neutrino

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