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Supernova relic neutrino search at super-Kamiokande

K. Bays6, T. Iida1, K. Abe1, Y. Hayato1,3, K. Iyogi1, J. Kameda1, Y. Koshio1, L. Marti1, M. Miura1 et al. (Super-Kamiokande Collaboration)

M. Miura1, S. Moriyama1,3, M. Nakahata1,3, S. Nakayama1, Y. Obayashi1, H. Sekiya1, M. Shiozawa1,3, Y. Suzuki1,3, A. Takeda1, Y. Takenaga1, K. Ueno1, K. Ueshima1, S. Yamada1, T. Yokozawa1, H. Kaji2, T. Kajita2,3, K. Kaneyuki2,3, T. McLachlan2, K. Okumura2, K. P. Lee2, K. Martens3, M. Vagins3,6, L. Labarga4, E. Kearns5,3, M. Litos5, J. L. Raaf5, J. L. Stone5,3, L. R. Sulak5, W. R. Kropp6, S. Mine6, C. Regis6, A. Renshaw6, M. B. Smy6,3, H. W. Sobel6,3, K. S. Ganezer7, J. Hill7, W. E. Keig7, S. Cho8, J. S. Jang8, J. Y. Kim8, I. T. Lim8, J. Albert9, K. Scholberg9,3, C. W. Walter9,3, R. Wendell9, T. Wongjirad9, T. Ishizuka10, S. Tasaka11, J. G. Learned12, S. Matsuno12, S. Smith12, T. Hasegawa13, T. Ishida13, T. Ishii13, T. Kobayashi13, T. Nakadaira13, K. Nakamura13,3, K. Nishikawa13, Y. Oyama13, K. Sakashita13, T. Sekiguchi13, T. Tsukamoto13, A. T. Suzuki14, Y. Takeuchi14,3, M. Ikeda15, K. Matsuoka15, A. Minamino15, A. Murakami15, T. Nakaya15,3, Y. Fukuda16, Y. Itow17, G. Mitsuka17, M. Miyake17, T. Tanaka17, J. Hignight18, J. Imber18, C. K. Jung18, I. Taylor18, C. Yanagisawa18, A. Kibayashi19, H. Ishino19, S. Mino19, M. Sakuda19, T. Mori19, H. Toyota19, Y. Kuno20, S. B. Kim21, B. S. Yang21, H. Okazawa22, Y. Choi23, K. Nishijima24, M. Koshiba25, Y. Totsuka25, M. Yokoyama25,3, Y. Heng26, S. Chen26, H. Zhang26, Z. Yang26, P. Mijakowski27, K. Connolly28, M. Dziomba28, and R. J. Wilkes28 (Super-Kamiokande Collaboration)

  • 1Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu, 506-1205, Japan
  • 2Research Center for Cosmic Neutrinos, Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba 277-8582, Japan
  • 3Institute for the Physics and Mathematics of the Universe, Todai Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba 277-8582, Japan
  • 4Department of Theoretical Physics, University Autonoma Madrid, 28049 Madrid, Spain
  • 5Department of Physics, Boston University, Boston, Massachusetts 02215, USA
  • 6Department of Physics and Astronomy, University of California, Irvine, Irvine, California 92697-4575, USA
  • 7Department of Physics, California State University, Dominguez Hills, Carson, California 90747, USA
  • 8Department of Physics, Chonnam National University, Kwangju 500-757, Korea
  • 9Department of Physics, Duke University, Durham, North Carolina 27708, USA
  • 10Junior College, Fukuoka Institute of Technology, Fukuoka, Fukuoka 811-0214, Japan
  • 11Department of Physics, Gifu University, Gifu, Gifu 501-1193, Japan
  • 12Department of Physics and Astronomy, University of Hawaii, Honolulu, Hawaii 96822, USA
  • 13High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan
  • 14Department of Physics, Kobe University, Kobe, Hyogo 657-8501, Japan
  • 15Department of Physics, Kyoto University, Kyoto, Kyoto 606-8502, Japan
  • 16Department of Physics, Miyagi University of Education, Sendai, Miyagi 980-0845, Japan
  • 17Solar Terrestrial Environment Laboratory, Nagoya University, Nagoya, Aichi 464-8602, Japan
  • 18Department of Physics and Astronomy, State University of New York, Stony Brook, New York 11794-3800, USA
  • 19Department of Physics, Okayama University, Okayama, Okayama 700-8530, Japan
  • 20Department of Physics, Osaka University, Toyonaka, Osaka 560-0043, Japan
  • 21Department of Physics, Seoul National University, Seoul 151-742, Korea
  • 22Department of Informatics in Social Welfare, Shizuoka University of Welfare, Yaizu, Shizuoka, 425-8611, Japan
  • 23Department of Physics, Sungkyunkwan University, Suwon 440-746, Korea
  • 24Department of Physics, Tokai University, Hiratsuka, Kanagawa 259-1292, Japan
  • 25The University of Tokyo, Bunkyo, Tokyo 113-0033, Japan
  • 26Department of Engineering Physics, Tsinghua University, Beijing, 100084, China
  • 27Institute of Experimental Physics, Warsaw University, 00-681 Warsaw, Poland
  • 28Department of Physics, University of Washington, Seattle, Washington 98195-1560, USA

Phys. Rev. D 85, 052007 – Published 22 March, 2012

DOI: https://doi.org/10.1103/PhysRevD.85.052007

Abstract

A new Super-Kamiokande search for supernova relic neutrinos was conducted using 2853 live days of data. Sensitivity is now greatly improved compared to the 2003 Super-Kamiokande result, which placed a flux limit near many theoretical predictions. This more detailed analysis includes a variety of improvements such as increased efficiency, a lower energy threshold, and an expanded data set. New combined upper limits on supernova relic neutrino flux are between 2.8 and 3.1ν¯ecm2s1>16MeV total positron energy (17.3 MeV Eν).

Article Text

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