Search for neutrinos in Super-Kamiokande associated with the GW170817 neutron-star merger
- Abe, K.
- Bronner, C.
- Hayato, Y.
- Ikeda, M.
- Iyogi, K.
- Kameda, J.
- Kato, Y.
- Kishimoto, Y.
- Marti, Ll.
- Miura, M.
- Moriyama, S.
- Nakahata, M.
- Nakajima, Y.
- Nakano, Y.
- Nakayama, S.
- Orii, A.
- Pronost, G.
- Sekiya, H.
- Shiozawa, M.
- Sonoda, Y.
- Takeda, A.
- Takenaka, A.
- Tanaka, H.
- Tasaka, S.
- Yano, T.
- Akutsu, R.
- Kajita, T.
- Nishimura, Y.
- Okumura, K.
- Tsui, K. M.
- Labarga, L.
- Fernandez, P.
- Blaszczyk, F. d. M.
- Kachulis, C.
- Kearns, E.
- Raaf, J. L.
- Stone, J. L.
- Sulak, L. R.
- Berkman, S.
- Tobayama, S.
- Bian, J.
- Elnimr, M.
- Kropp, W. R.
- Locke, S.
- Mine, S.
- Weatherly, P.
- Smy, M. B.
- Sobel, H. W.
- Takhistov, V.
- Ganezer, K. S.
- Hill, J.
- Kim, J. Y.
- Lim, I. T.
- Park, R. G.
- Li, Z.
- O’Sullivan, E.
- Scholberg, K.
- Walter, C. W.
- Gonin, M.
- Imber, J.
- Mueller, Th. A.
- Ishizuka, T.
- Nakamura, T.
- Jang, J. S.
- Choi, K.
- Learned, J. G.
- Matsuno, S.
- Amey, J.
- Litchfield, R. P.
- Ma, W. Y.
- Uchida, Y.
- Wascko, M. O.
- Catanesi, M. G.
- Intonti, R. A.
- Radicioni, E.
- Rosa, G. De
- Ali, A.
- Collazuol, G.
- Ludovici, L.
- Cao, S.
- Friend, M.
- Hasegawa, T.
- Ishida, T.
- Ishii, T.
- Kobayashi, T.
- Nakadaira, T.
- Nakamura, K.
- Oyama, Y.
- Sakashita, K.
- Sekiguchi, T.
- Tsukamoto, T.
- Abe, KE.
- Hasegawa, M.
- Suzuki, A. T.
- Takeuchi, Y.
- Hayashino, T.
- Hirota, S.
- Jiang, M.
- Mori, M.
- Nakamura, KE.
- Nakaya, T.
- Wendell, R. A.
- Anthony, L. H. V.
- McCauley, N.
- Pritchard, A.
- Fukuda, Y.
- Itow, Y.
- Murase, M.
- Muto, F.
- Mijakowski, P.
- Frankiewicz, K.
- Jung, C. K.
- Li, X.
- Palomino, J. L.
- Santucci, G.
- Viela, C.
- Wilking, M. J.
- Yanagisawa, C.
- Fukuda, D.
- Ishino, H.
- Ito, S.
- Kibayashi, A.
- Koshio, Y.
- Nagata, H.
- Sakuda, M.
- Xu, C.
- Kuno, Y.
- Wark, D.
- Lodovico, F. Di
- Richards, B.
- Sedgwick, S. Molina
- Tacik, R.
- Kim, S. B.
- Cole, A.
- Thompson, L.
- Okazawa, H.
- Choi, Y.
- Ito, K.
- Nishijima, K.
- Koshiba, M.
- Suda, Y.
- Yokoyama, M.
- Calland, R. G.
- Hartz, M.
- Martens, K.
- Murdoch, M.
- Quilain, B.
- Simpson, C.
- Suzuki, Y.
- Vagins, M. R.
- Hamabe, D.
- Kuze, M.
- Okajima, Y.
- Yoshida, T.
- Ishitsuka, M.
- Martin, J. F.
- Nantais, C. M.
- Tanaka, H. A.
- Towstego, T.
- Konaka, A.
- Chen, S.
- Wan, L.
- Minamino, A.
DOIAbstract
We report the results of a neutrino search in Super-Kamiokande (SK) for coincident signals with the first detected gravitational wave (GW) produced by a binary neutron-star merger, GW170817, which was followed by a short gamma-ray burst, GRB170817A, and a kilonova/macronova. We searched for coincident neutrino events in the range from 3.5 MeV to ~100 PeV, in a time window ±500 s around the gravitational wave detection time, as well as during a 14-day period after the detection. No significant neutrino signal was observed for either time window. We calculated 90% confidence level upper limits on the neutrino fluence for GW170817. From the upward-going-muon events in the energy region above 1.6 GeV, the neutrino fluence limit is ${16.0}_{-0.6...
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