Search for tens of MeV neutrinos associated with gamma-ray bursts in Super-Kamiokande,Progress of Theoretical and Experimental Physics

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Search for tens of MeV neutrinos associated with gamma-ray bursts in Super-Kamiokande
Progress of Theoretical and Experimental Physics Pub Date : 2021-07-02 , DOI: 10.1093/ptep/ptab081
A Orii ₁ , K Abe _{1,

2} , C Bronner ₁ , Y Hayato _{1,

2} , M Ikeda ₁ , S Imaizumi ₁ , H Ito ₁ , J Kameda _{1,

2} , Y Kataoka ₁ , Y Kato ₁ , Y Kishimoto _{1,

2} , M Miura ₁ , S Moriyama _{1,

2} , T Mochizuki ₁ , Y Nagao ₁ , M Nakahata _{1,

2} , Y Nakajima _{1,

2} , S Nakayama _{1,

2} , T Okada ₁ , K Okamoto ₁ , G Pronost ₁ , H Sekiya _{1,

2} , M Shiozawa _{1,

2} , Y Sonoda ₁ , Y Suzuki ₁ , A Takeda _{1,

2} , Y Takemoto ₁ , A Takenaka ₁ , H Tanaka ₁ , T Yano ₁ , S Han ₃ , T Kajita _{2,

3} , K Okumura _{2,

3} , T Tashiro ₃ , R Wang ₃ , J Xia ₃ , G D Megias ₄ , D Bravo-Berguño ₅ , L Labarga ₅ , Ll Marti ₅ , B Zaldivar ₅ , F d M Blaszczyk ₆ , E Kearns _{2,

6} , J L Raaf ₆ , J L Stone _{2,

6} , L Wan ₆ , T Wester ₆ , B W Pointon ₇ , J Bian ₈ , N J Griskevich ₈ , W R Kropp ₈ , S Locke ₈ , S Mine ₈ , M B Smy _{2,

8} , H W Sobel _{2,

8} , V Takhistov _{2,

8} , P Weatherly ₈ , K S Ganezer ₉ , J Hill ₉ , J Y Kim ₁₀ , I T Lim ₁₀ , R G Park ₁₀ , B Bodur ₁₁ , K Scholberg _{2,

11} , C W Walter _{2,

11} , L Bernard ₁₂ , A Coffani ₁₂ , O Drapier ₁₂ , S El Hedri ₁₂ , A Giampaolo ₁₂ , M Gonin ₁₂ , Th A Mueller ₁₂ , P Paganini ₁₂ , B Quilain ₁₂ , T Ishizuka ₁₃ , T Nakamura ₁₄ , J S Jang ₁₅ , J G Learned ₁₆ , S Matsuno ₁₆ , L H V Anthony ₁₇ , R P Litchfield ₁₇ , A A Sztuc ₁₇ , Y Uchida ₁₇ , V Berardi ₁₈ , M G Catanesi ₁₈ , E Radicioni ₁₈ , N F Calabria ₁₉ , L N Machado ₁₉ , G De Rosa ₁₉ , G Collazuol ₂₀ , F Iacob ₂₀ , M Lamoureux ₂₀ , N Ospina ₂₀ , L Ludovici ₂₁ , Y Nishimura ₂₂ , S Cao ₂₃ , M Friend ₂₃ , T Hasegawa ₂₃ , T Ishida ₂₃ , T Kobayashi ₂₃ , M Jakkapu ₂₃ , T Matsubara ₂₃ , T Nakadaira ₂₃ , K Nakamura _{2,

23} , Y Oyama ₂₃ , K Sakashita ₂₃ , T Sekiguchi ₂₃ , T Tsukamoto ₂₃ , T Boschi ₂₄ , F Di Lodovico ₂₄ , S Molina Sedgwick ₂₄ , M Taani ₂₄ , S Zsoldos ₂₄ , M Hasegawa ₂₅ , Y Isobe ₂₅ , H Miyabe ₂₅ , Y Nakano ₂₅ , T Shiozawa ₂₅ , T Sugimoto ₂₅ , A T Suzuki ₂₅ , Y Takeuchi _{2,

25} , S Yamamoto ₂₅ , A Ali ₂₆ , Y Ashida ₂₆ , J Feng ₂₆ , S Hirota ₂₆ , M Jiang ₂₆ , A K Ichikawa ₂₆ , T Kikawa ₂₆ , M Mori ₂₆ , K E Nakamura ₂₆ , T Nakaya _{2,

26} , R A Wendell _{2,

26} , K Yasutome ₂₆ , P Fernandez ₂₇ , N McCauley ₂₇ , P Mehta ₂₇ , A Pritchard ₂₇ , K M Tsui ₂₇ , Y Fukuda ₂₈ , Y Itow _{29,

30} , H Menjo ₂₉ , T Niwa ₂₉ , K Sato ₂₉ , M Tsukada ₂₉ , P Mijakowski ₃₁ , K Frankiewicz ₃₁ , C K Jung ₃₂ , C Vilela ₃₂ , M J Wilking ₃₂ , C Yanagisawa ₃₂ , D Fukuda ₃₃ , M Harada ₃₃ , K Hagiwara ₃₃ , T Horai ₃₃ , H Ishino ₃₃ , S Ito ₃₃ , Y Koshio _{2,

33} , W Ma ₃₃ , N Piplani ₃₃ , S Sakai ₃₃ , M Sakuda ₃₃ , Y Takahira ₃₃ , C Xu ₃₃ , Y Kuno ₃₄ , G Barr ₃₅ , D Barrow ₃₅ , L Cook _{2,

35} , A Goldsack _{2,

35} , S Samani ₃₅ , C Simpson _{2,

35} , D Wark _{35,

36} , F Nova ₃₇ , J Y Yang ₃₈ , S J Jenkins ₃₉ , M Malek ₃₉ , J M McElwee ₃₉ , O Stone ₃₉ , M D Thiesse ₃₉ , L F Thompson ₃₉ , H Okazawa ₄₀ , Y Choi ₄₁ , S B Kim ₄₁ , I Yu ₄₁ , K Nishijima ₄₂ , M Koshiba ₄₃ , K Iwamoto ₄₄ , N Ogawa ₄₄ , M Yokoyama _{2,

44} , K Martens ₂ , M R Vagins _{2,

8} , S Izumiyama ₄₅ , M Kuze ₄₅ , M Tanaka ₄₅ , T Yoshida ₄₅ , M Inomoto ₄₆ , M Ishitsuka ₄₆ , R Matsumoto ₄₆ , K Ohta ₄₆ , M Shinoki ₄₆ , J F Martin ₄₇ , C M Nantais ₄₇ , H A Tanaka ₄₇ , T Towstego ₄₇ , R Akutsu ₄₈ , M Hartz _{2,

48} , A Konaka ₄₈ , P de Perio ₄₈ , N W Prouse ₄₈ , S Chen ₄₉ , B D Xu ₄₉ , M Posiadala-Zezula ₅₀ , B Richards ₅₁ , B Jamieson ₅₂ , J Walker ₅₂ , A Minamino ₅₃ , K Okamoto ₅₃ , G Pintaudi ₅₃ , R Sasaki ₅₃

Affiliation

Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan
Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba 277-8583, Japan
Research Center for Cosmic Neutrinos, Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba 277-8582, Japan
Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba 277-8582, Japan
Department of Theoretical Physics, University Autonoma Madrid, 28049 Madrid, Spain
Department of Physics, Boston University, Boston, MA 02215, USA
Department of Physics, British Columbia Institute of Technology, Burnaby, BC, V5G 3H2, Canada
Department of Physics and Astronomy, University of California, Irvine, Irvine, CA 92697-4575, USA
Department of Physics, California State University, Dominguez Hills, Carson, CA 90747, USA
Institute for Universe and Elementary Particles, Chonnam National University, Gwangju 61186, Korea
Department of Physics, Duke University, Durham NC 27708, USA
Ecole Polytechnique, IN2P3-CNRS, Laboratoire Leprince-Ringuet, F-91120 Palaiseau, France
Junior College, Fukuoka Institute of Technology, Fukuoka, Fukuoka 811-0295, Japan
Department of Physics, Gifu University, Gifu, Gifu 501-1193, Japan
GIST College, Gwangju Institute of Science and Technology, Gwangju 500-712, Korea
Department of Physics and Astronomy, University of Hawaii, Honolulu, HI 96822, USA
Department of Physics, Imperial College London, London, SW7 2AZ, United Kingdom
Dipartimento Interuniversitario di Fisica, INFN Sezione di Bari and Università e Politecnico di Bari, I-70125, Bari, Italy
Dipartimento di Fisica, INFN Sezione di Napoli and Università di Napoli, I-80126, Napoli, Italy
Dipartimento di Fisica, INFN Sezione di Padova and Università di Padova, I-35131, Padova, Italy
INFN Sezione di Roma and Università di Roma “La Sapienza,” I-00185, Roma, Italy
Department of Physics, Keio University, Yokohama, Kanagawa, 223-8522, Japan
High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan
Department of Physics, King’s College London, London, WC2R 2LS, UK
Department of Physics, Kobe University, Kobe, Hyogo 657-8501, Japan
Department of Physics, Kyoto University, Kyoto, Kyoto 606-8502, Japan
Department of Physics, University of Liverpool, Liverpool, L69 7ZE, United Kingdom
Department of Physics, Miyagi University of Education, Sendai, Miyagi 980-0845, Japan
Institute for Space-Earth Environmental Research, Nagoya University, Nagoya, Aichi 464-8602, Japan
Kobayashi-Maskawa Institute for the Origin of Particles and the Universe, Nagoya University, Nagoya, Aichi 464-8602, Japan
National Centre For Nuclear Research, 02-093 Warsaw, Poland
Department of Physics and Astronomy, State University of New York at Stony Brook, NY 11794-3800, USA
Department of Physics, Okayama University, Okayama, Okayama 700-8530, Japan
Department of Physics, Osaka University, Toyonaka, Osaka 560-0043, Japan
Department of Physics, Oxford University, Oxford, OX1 3PU, United Kingdom
STFC, Rutherford Appleton Laboratory, Harwell, Oxford, and Daresbury Laboratory, Warrington, OX11 0QX, United Kingdom
Rutherford Appleton Laboratory, Harwell, Oxford, OX11 0QX, UK
Department of Physics, Seoul National University, Seoul 151-742, Korea
Department of Physics and Astronomy, University of Sheffield, S3 7RH, Sheffield, United Kingdom
Department of Informatics in Social Welfare, Shizuoka University of Welfare, Yaizu, Shizuoka, 425-8611, Japan
Department of Physics, Sungkyunkwan University, Suwon 440-746, Korea
Department of Physics, Tokai University, Hiratsuka, Kanagawa 259-1292, Japan
The University of Tokyo, Bunkyo, Tokyo 113-0033, Japan
Department of Physics, University of Tokyo, Bunkyo, Tokyo 113-0033, Japan
Department of Physics, Tokyo Institute of Technology, Meguro, Tokyo 152-8551, Japan
Department of Physics, Faculty of Science and Technology, Tokyo University of Science, Noda, Chiba 278-8510, Japan
Department of Physics, University of Toronto, ON, M5S 1A7, Canada
TRIUMF, 4004 Wesbrook Mall, Vancouver, BC, V6T2A3, Canada
Department of Engineering Physics, Tsinghua University, Beijing, 100084, China
Faculty of Physics, University of Warsaw, Warsaw, 02-093, Poland
Department of Physics, University of Warwick, Coventry, CV4 7AL, UK
Department of Physics, University of Winnipeg, MB R3J 3L8, Canada
Department of Physics, Yokohama National University, Yokohama, Kanagawa, 240-8501, Japan

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 |$\bar\nu_e$| fluence in the range from 8 MeV to 100 MeV in positron total energy for |$\bar\nu_e+p\rightarrow e^{+}+n$| was found to be less than |$\rm 5.07\times10^5$| 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.

中文翻译：

在超级神冈中寻找与伽马射线爆发相关的数十个 MeV 中微子

使用超级神冈 (SK) 探测器对与伽马射线暴 (GRB) 一致产生的中微子进行了搜索。2008 年 12 月至 2017 年 3 月期间，伽马射线坐标网络记录了 2208 次 SK 正常运行期间发生的 GRB。每个 GRB 周围的几个时间窗口被用来搜索重合的中微子事件。没有检测到超过估计背景的统计显着信号。该| $ \酒吧\ nu_e $ | |$\bar\nu_e+p\rightarrow e^{+}+n$| 的正电子总能量范围为 8 MeV 到 100 MeV 发现小于|$\rm 5.07\times10^5$| 厘米|$^{-2}$|每个 GRB 在 90% 的置信水平。对于所有 GRB，根据中微子能量获得了注量的上限。此外，对于已知距离处的 GRB，为 GRB 处的中微子能量发射设定了上限。

更新日期：2021-07-02

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