文献类型：期刊文献

英文题名：Search for electron-antineutrinos associated with gravitational-wave events GW150914, GW151012, GW151226, GW170104, GW170608, GW170814, and GW170817 at Daya Bay

作者：An, F.P.[1]; Balantekin, A.B.[2]; Band, H.R.[3]; Bishai, M.[4]; Blyth, S.[5]; Cao, G.F.[6]; Cao, J.[6]; Chang, J.F.[6]; Chang, Y.[7]; Chen, H.S.[6]; Chen, S.M.[8]; Chen, Y.[9,10]; Chen, Y.X.[11]; Cheng, J.[6]; Cheng, Z.K.[10]; Cherwinka, J.J.[2]; Chu, M.C.[12]; Cummings, J.P.[13]; Dalager, O.[14]; Deng, F.S.[15]; Ding, Y.Y.[6]; Diwan, M.V.[4]; Dohnal, T.[16]; Dove, J.[17]; Dvo?ák, M.[16]; Dwyer, D.A.[18]; Gallo, J.P.[19]; Gonchar, M.[20]; Gong, G.H.[8]; Gong, H.[8]; Gu, W.Q.[4]; Guo, J.Y.[10]; Guo, L.[8]; Guo, X.H.[21]; Guo, Y.H.[22]; Guo, Z.[8]; Hackenburg, R.W.[4]; Hans, S.[4]; He, M.[6]; Heeger, K.M.[3]; Heng, Y.K.[6]; Higuera, A.[23]; Hor, Y.K.[10]; Hsiung, Y.B.[5]; Hu, B.Z.[5]; Hu, J.R.[6]; Hu, T.[6]; Hu, Z.J.[10]; Huang, H.X.[24]; Huang, X.T.[25]; Huang, Y.B.[26]; Huber, P.[27]; Jaffe, D.E.[4]; Jen, K.L.[28]; Ji, X.L.[6]; Ji, X.P.[4]; Johnson, R.A.[29]; Jones, D.[30]; Kang, L.[31]; Kettell, S.H.[4]; Kohn, S.[32]; Kramer, M.[18,32]; Langford, T.J.[3]; Lee, J.[18]; Lee, J.H.C.[33]; Lei, R.T.[31]; Leitner, R.[16]; Leung, J.K.C.[33]; Li, F.[6]; Li, J.J.[8]; Li, Q.J.[6]; Li, S.[31]; Li, S.C.[27]; Li, W.D.[6]; Li, X.N.[6]; Li, X.Q.[34]; Li, Y.F.[6]; Li, Z.B.[10]; Liang, H.[15]; Lin, C.J.[18]; Lin, G.L.[28]; Lin, S.[31]; Ling, J.J.[10]; Link, J.M.[27]; Littenberg, L.[4]; Littlejohn, B.R.[19]; Liu, J.C.[6]; Liu, J.L.[35]; Lu, C.[36]; Lu, H.Q.[6]; Lu, J.S.[6]; Luk, K.B.[18,32]; Ma, X.B.[11]; Ma, X.Y.[6]; Ma, Y.Q.[6]; Marshall, C.[18]; Martinez Caicedo, D.A.[19]; McDonald, K.T.[36]; McKeown, R.D.[37,38]; Meng, Y.[35]; Napolitano, J.[30]; Naumov, D.[20]; Naumova, E.[20]; Ochoa-Ricoux, J.P.[14]; Olshevskiy, A.[20]; Pan, H.-R.[5]; Park, J.[27]; Patton, S.[18]; Peng, J.C.[17]; Pun, C.S.J.[33]; Qi, F.Z.[6]; Qi, M.[39]; Qian, X.[4]; Raper, N.[10]; Ren, J.[24]; Morales Reveco, C.[14]; Rosero, R.[4]; Roskovec, B.[14]; Ruan, X.C.[24]; Steiner, H.[18,32]; Sun, J.L.[40]; Tmej, T.[16]; Treskov, K.[20]; Tse, W.-H.[12]; Tull, C.E.[18]; Viren, B.[4]; Vorobel, V.[16]; Wang, C.H.[7]; Wang, J.[10]; Wang, M.[25]; Wang, N.Y.[21]; Wang, R.G.[6]; Wang, W.[10,38]; Wang, W.[39]; Wang, X.[41]; Wang, Y.[39]; Wang, Y.F.[6]; Wang, Z.[6]; Wang, Z.[8]; Wang, Z.M.[6]; Wei, H.Y.[4]; Wei, L.H.[6]; Wen, L.J.[6]; Whisnant, K.[42]; White, C.G.[19]; Wong, H.L.H.[18,32]; Worcester, E.[4]; Wu, D.R.[6]; Wu, F.L.[39]; Wu, Q.[25]; Wu, W.J.[6]; Xia, D.M.[43]; Xie, Z.Q.[6]; Xing, Z.Z.[6]; Xu, J.L.[6]; Xu, T.[8]; Xue, T.[8]; Yang, C.G.[6]; Yang, L.[31]; Yang, Y.Z.[8]; Yao, H.F.[6]; Ye, M.[6]; Yeh, M.[4]; Young, B.L.[42]; Yu, H.Z.[10]; Yu, Z.Y.[6]; Yue, B.B.[10]; Zeng, S.[6]; Zeng, Y.[10]; Zhan, L.[6]; Zhang, C.[4]; Zhang, F.Y.[35]

机构：[1] Institute of Modern Physics, East China University of Science and Technology, Shanghai, China; [2] University of Wisconsin, Madison, WI, 53706, United States; [3] Wright Laboratory and Department of Physics, Yale University, New Haven, CT, 06520, United States; [4] Brookhaven National Laboratory, Upton, NY, 11973, United States; [5] Department of Physics, National Taiwan University, Taipei, Taiwan; [6] Institute of High Energy Physics, Beijing, China; [7] National United University, Miao-Li, Taiwan; [8] Department of Engineering Physics, Tsinghua University, Beijing, China; [9] Shenzhen University, Shenzhen, China; [10] Sun Yat-Sen [Zhongshan] University, Guangzhou, China; [11] North China Electric Power University, Beijing, China; [12] Chinese University of Hong Kong, Hong Kong; [13] Siena College, Loudonville, NY, 12211, United States; [14] Department of Physics and Astronomy, University of California, Irvine, CA, 92697, United States; [15] University of Science and Technology of China, Hefei, China; [16] Charles University, Faculty of Mathematics and Physics, Prague, Czech Republic; [17] Department of Physics, University of Illinois at Urbana-Champaign, Urbana, IL, 61801, United States; [18] Lawrence Berkeley National Laboratory, Berkeley, CA, 94720, United States; [19] Department of Physics, Illinois Institute of Technology, Chicago, IL, 60616, United States; [20] Joint Institute for Nuclear Research, Moscow Region, Dubna, Russia; [21] Beijing Normal University, Beijing, China; [22] Department of Nuclear Science and Technology, School of Energy and Power Engineering, Xi’an Jiaotong University, Xi’an, China; [23] Department of Physics, University of Houston, Houston, TX, 77204, United States; [24] China Institute of Atomic Energy, Beijing, China; [25] Shandong University, Jinan, China; [26] Guangxi University, Nanning, China; [27] Center for Neutrino Physics, Virginia Tech, Blacksburg, VA, 24061, United States; [28] Institute of Physics, National Chiao-Tung University, Hsinchu, Taiwan; [29] Department of Physics, University of Cincinnati, Cincinnati, OH, 45221, United States; [30] Department of Physics, College of Science and Technology, Temple University, Philadelphia, PA, 19122, United States; [31] Dongguan University of Technology, Dongguan, China; [32] Department of Physics, University of California, Berkeley, CA, 94720, United States; [33] Department of Physics, The University of Hong Kong, Pokfulam, Hong Kong; [34] School of Physics, Nankai University, Tianjin, China; [35] Department of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai Laboratory for Particle Physics and Cosmology, Shanghai, China; [36] Joseph Henry Laboratories, Princeton University, Princeton, NJ, 08544, United States; [37] California Institute of Technology, Pasadena, CA, 91125, United States; [38] College of William and Mary, Williamsburg, VA, 23187, United States; [39] Nanjing University, Nanjing, China; [40] China General Nuclear Power Group, Shenzhen, China; [41] College of Electronic Science and Engineering, National University of Defense Technology, Changsha, China; [42] Iowa State University, Ames, IA, 50011, United States; [43] Chongqing University, Chongqing, China

年份：2020

外文期刊名：arXiv

收录：EI(收录号：20200566141)

语种：英文

外文关键词：Black holes - Electrons - Gravitational effects - Neutrons - Stars

摘要：Providing a possible connection between neutrino emission and gravitational-wave (GW) bursts is important to our understanding of the physical processes that occur when black holes or neutron stars merge. In the Daya Bay experiment, using the data collected from December 2011 to August 2017, a search has been performed for electron-antineutrino signals coinciding with detected GW events, including GW150914, GW151012, GW151226, GW170104, GW170608, GW170814, and GW170817. We used three time windows of ±10 s, ±500 s, and ±1000 s relative to the occurrence of the GW events, and a neutrino energy range of 1.8 to 100 MeV to search for correlated neutrino candidates. The detected electron-antineutrino candidates are consistent with the expected background rates for all the three time windows. Assuming monochromatic spectra, we found upper limits (90% confidence level) on electron-antineutrino fluence of (1.13 ? 2.44)×1011 cm?2 at 5 MeV to 8.0×107 cm?2 at 100 MeV for the three time windows. Under the assumption of a Fermi-Dirac spectrum, the upper limits were found to be (5.4 ? 7.0)×109 cm?2 for the three time windows. Copyright ? 2020, The Authors. All rights reserved.