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Search for tens of MeV neutrinos associated with gamma-ray bursts in Super-Kamiokandeopen access

Authors
Orii, A.[Orii, A.]Abe, K.[Abe, K.]Bronner, C.[Bronner, C.]Hayato, Y.[Hayato, Y.]Ikeda, M.[Ikeda, M.]Imaizumi, S.[Imaizumi, S.]Ito, H.[Ito, H.]Kameda, J.[Kameda, J.]Kataoka, Y.[Kataoka, Y.]Kato, Y.[Kato, Y.]Kishimoto, Y.[Kishimoto, Y.]Miura, M.[Miura, M.]Moriyama, S.[Moriyama, S.]Mochizuki, T.[Mochizuki, T.]Nagao, Y.[Nagao, Y.]Nakahata, M.[Nakahata, M.]Nakajima, Y.[Nakajima, Y.]Nakayama, S.[Nakayama, S.]Okada, T.[Okada, T.]Okamoto, K.[Okamoto, K.]Pronost, G.[Pronost, G.]Sekiya, H.[Sekiya, H.]Shiozawa, M.[Shiozawa, M.]Sonoda, Y.[Sonoda, Y.]Suzuki, Y.[Suzuki, Y.]Takeda, A.[Takeda, A.]Takemoto, Y.[Takemoto, Y.]Takenaka, A.[Takenaka, A.]Tanaka, H.[Tanaka, H.]Yano, T.[Yano, T.]Han, S.[Han, S.]Kajita, T.[Kajita, T.]Okumura, K.[Okumura, K.]Tashiro, T.[Tashiro, T.]Wang, R.[Wang, R.]Xia, J.[Xia, J.]Megias, G.D.[Megias, G.D.]Bravo-Berguño, D.[Bravo-Berguño, D.]Labarga, L.[Labarga, L.]Marti, L.[Marti, L.]Zaldivar, B.[Zaldivar, B.]Blaszczyk, F.D.M.[Blaszczyk, F.D.M.]Kearns, E.[Kearns, E.]Raaf, J.L.[Raaf, J.L.]Stone, J.L.[Stone, J.L.]Wan, L.[Wan, L.]Wester, T.[Wester, T.]Pointon, B.W.[Pointon, B.W.]Bian, J.[Bian, J.]Griskevich, N.J.[Griskevich, N.J.]Kropp, W.R.[Kropp, W.R.]Locke, S.[Locke, S.]Mine, S.[Mine, S.]Smy, M.B.[Smy, M.B.]Sobel, H.W.[Sobel, H.W.]Takhistov, V.[Takhistov, V.]Weatherly, P.[Weatherly, P.]Ganezer, K.S.[Ganezer, K.S.]Hill, J.[Hill, J.]Kim, J.Y.[Kim, J.Y.]Lim, I.T.[Lim, I.T.]Park, R.G.[Park, R.G.]Bodur, B.[Bodur, B.]Scholberg, K.[Scholberg, K.]Walter, C.W.[Walter, C.W.]Bernard, L.[Bernard, L.]Coffani, A.[Coffani, A.]Drapier, O.[Drapier, O.]El, Hedri S.[El, Hedri S.]Giampaolo, A.[Giampaolo, A.]Gonin, M.[Gonin, M.]Mueller, T.A.[Mueller, T.A.]Paganini, P.[Paganini, P.]Quilain, B.[Quilain, B.]Ishizuka, T.[Ishizuka, T.]Nakamura, T.[Nakamura, T.]Jang, J.S.[Jang, J.S.]Learned, J.G.[Learned, J.G.]Matsuno, S.[Matsuno, S.]Anthony, L.H.V.[Anthony, L.H.V.]Litchfield, R.P.[Litchfield, R.P.]Sztuc, A.A.[Sztuc, A.A.]Uchida, Y.[Uchida, Y.]Berardi, V.[Berardi, V.]Catanesi, M.G.[Catanesi, M.G.]Radicioni, E.[Radicioni, E.]Calabria, N.F.[Calabria, N.F.]Machado, L.N.[Machado, L.N.]De, Rosa G.[De, Rosa G.]Collazuol, G.[Collazuol, G.]Iacob, F.[Iacob, F.]Lamoureux, M.[Lamoureux, M.]Ospina, N.[Ospina, N.]Ludovici, L.[Ludovici, L.]Nishimura, Y.[Nishimura, Y.]Cao, S.[Cao, S.]Friend, M.[Friend, M.]Hasegawa, T.[Hasegawa, T.]Ishida, T.[Ishida, T.]Kobayashi, T.[Kobayashi, T.]Jakkapu, M.[Jakkapu, M.]Matsubara, T.[Matsubara, T.]Nakadaira, T.[Nakadaira, T.]Nakamura, K.[Nakamura, K.]Oyama, Y.[Oyama, Y.]Sakashita, K.[Sakashita, K.]Sekiguchi, T.[Sekiguchi, T.]Tsukamoto, T.[Tsukamoto, T.]Boschi, T.[Boschi, T.]Di, Lodovico F.[Di, Lodovico F.]Sedgwick, S.M.[Sedgwick, S.M.]Taani, M.[Taani, M.]Zsoldos, S.[Zsoldos, S.]Hasegawa, M.[Hasegawa, M.]Isobe, Y.[Isobe, Y.]Miyabe, H.[Miyabe, H.]Nakano, Y.[Nakano, Y.]Shiozawa, T.[Shiozawa, T.]Sugimoto, T.[Sugimoto, T.]Suzuki, A.T.[Suzuki, A.T.]Takeuchi, Y.[Takeuchi, Y.]Yamamoto, S.[Yamamoto, S.]Ali, A.[Ali, A.]Ashida, Y.[Ashida, Y.]Feng, J.[Feng, J.]Hirota, S.[Hirota, S.]Jiang, M.[Jiang, M.]Ichikawa, A.K.[Ichikawa, A.K.]Kikawa, T.[Kikawa, T.]Mori, M.[Mori, M.]Nakamura, K.E.[Nakamura, K.E.]Nakaya, T.[Nakaya, T.]Wendell, R.A.[Wendell, R.A.]Yasutome, K.[Yasutome, K.]Fernandez, P.[Fernandez, P.]Mccauley, N.[Mccauley, N.]Mehta, P.[Mehta, P.]Pritchard, A.[Pritchard, A.]Tsui, K.M.[Tsui, K.M.]Fukuda, Y.[Fukuda, Y.]Itow, Y.[Itow, Y.]Menjo, H.[Menjo, H.]Niwa, T.[Niwa, T.]Sato, K.[Sato, K.]Tsukada, M.[Tsukada, M.]Mijakowski, P.[Mijakowski, P.]Frankiewicz, K.[Frankiewicz, K.]Jung, C.K.[Jung, C.K.]Vilela, C.[Vilela, C.]Wilking, M.J.[Wilking, M.J.]Yanagisawa, C.[Yanagisawa, C.]Fukuda, D.[Fukuda, D.]Harada, M.[Harada, M.]Hagiwara, K.[Hagiwara, K.]Horai, T.[Horai, T.]Ishino, H.[Ishino, H.]Ito, S.[Ito, S.]Koshio, Y.[Koshio, Y.]Ma, W.[Ma, W.]Piplani, N.[Piplani, N.]Sakai, S.[Sakai, S.]Sakuda, M.[Sakuda, M.]Takahira, Y.[Takahira, Y.]Xu, C.[Xu, C.]Kuno, Y.[Kuno, Y.]Barr, G.[Barr, G.]Barrow, D.[Barrow, D.]Cook, L.[Cook, L.]Goldsack, A.[Goldsack, A.]Samani, S.[Samani, S.]Simpson, C.[Simpson, C.]Wark, D.[Wark, D.]Nova, F.[Nova, F.]Yang, J.Y.[Yang, J.Y.]Jenkins, S.J.[Jenkins, S.J.]Malek, M.[Malek, M.]Mcelwee, J.M.[Mcelwee, J.M.]Stone, O.[Stone, O.]Thiesse, M.D.[Thiesse, M.D.]Thompson, L.F.[Thompson, L.F.]Okazawa, H.[Okazawa, H.]Choi, Y.[Choi, Y.]Kim, S.B.[Kim, S.B.]Yu, I.[Yu, I.]Nishijima, K.[Nishijima, K.]Koshiba, M.[Koshiba, M.]Iwamoto, K.[Iwamoto, K.]Ogawa, N.[Ogawa, N.]Yokoyama, M.[Yokoyama, M.]Martens, K.[Martens, K.]Vagins, M.R.[Vagins, M.R.]Izumiyama, S.[Izumiyama, S.]Kuze, M.[Kuze, M.]Tanaka, M.[Tanaka, M.]Yoshida, T.[Yoshida, T.]Inomoto, M.[Inomoto, M.]Ishitsuka, M.[Ishitsuka, M.]Matsumoto, R.[Matsumoto, R.]Ohta, K.[Ohta, K.]Shinoki, M.[Shinoki, M.]Martin, J.F.[Martin, J.F.]Nantais, C.M.[Nantais, C.M.]Tanaka, H.A.[Tanaka, H.A.]Towstego, T.[Towstego, T.]Akutsu, R.[Akutsu, R.]Hartz, M.[Hartz, M.]Konaka, A.[Konaka, A.]De, Perio P.[De, Perio P.]Prouse, N.W.[Prouse, N.W.]Chen, S.[Chen, S.]Xu, B.D.[Xu, B.D.]Posiadala-Zezula, M.[Posiadala-Zezula, M.]Richards, B.[Richards, B.]Jamieson, B.[Jamieson, B.]Walker, J.[Walker, J.]Minamino, A.[Minamino, A.]Okamoto, K.[Okamoto, K.]Pintaudi, G.[Pintaudi, G.]Sasaki, R.[Sasaki, R.]Super-Kamiokande Collaboration[Super-Kamiokande Collaboration]
Issue Date
7-Oct-2021
Publisher
Physical Society of Japan
Citation
Progress of Theoretical and Experimental Physics, v.2021, no.10
Indexed
SCIE
SCOPUS
Journal Title
Progress of Theoretical and Experimental Physics
Volume
2021
Number
10
URI
https://scholarworks.bwise.kr/skku/handle/2021.sw.skku/90969
DOI
10.1093/ptep/ptab081
ISSN
2050-3911
Abstract
A search for neutrinos produced in coincidence with gamma-ray bursts (GRBs) was conducted with the Super-Kamiokande (SK) detector. Between December 2008 and March 2017, the Gamma-ray Coordinates Network recorded 2208 GRBs that occurred during normal SK operation. Several time windows around each GRB were used to search for coincident neutrino events. No statistically significant signal in excess of the estimated backgrounds was detected. The νe fluence in the range from 8 MeV to 100 MeV in positron total energy for νe+p → e++n was found to be less than 5.07 × 105 cm-2 per GRB at a 90% confidence level. For all GRBs, upper bounds were obtained on the fluence as a function of neutrino energy. Additionally, for GRBs at known distances, upper limits were set for the neutrino energy emission at the GRB. © 2021 The Author(s). Published by Oxford University Press on behalf of the Physical Society of Japan.
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