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

被引：0

作者：

F.P.An ^{[1
]}

A.B.Balantekin ^{[2
]}

H.R.Band ^{[3
]}

M.Bishai ^{[4
]}

S.Blyth ^{[5
]}

G.F.Cao ^{[6
]}

J.Cao ^{[6
]}

J.F.Chang ^{[6
]}

Y.Chang ^{[7
]}

H.S.Chen ^{[6
]}

S.M.Chen ^{[8
]}

Y.Chen ^{[9
,10
]}

Y.X.Chen ^{[11
]}

J.Cheng ^{[6
]}

Z.K.Cheng ^{[10
]}

J.J.Cherwinka ^{[2
]}

M.C.Chu ^{[12
]}

J.P.Cummings ^{[13
]}

O.Dalager ^{[14
]}

F.S.Deng ^{[15
]}

Y.Y.Ding ^{[6
]}

M.V.Diwan ^{[4
]}

T.Dohnal ^{[16
]}

J.Dove ^{[17
]}

M.Dvo?ák ^{[16
]}

D.A.Dwyer ^{[18
]}

J.P.Gallo ^{[19
]}

M.Gonchar ^{[20
]}

G.H.Gong ^{[8
]}

H.Gong ^{[8
]}

W.Q.Gu ^{[4
]}

J.Y.Guo ^{[10
]}

L.Guo ^{[8
]}

X.H.Guo ^{[21
]}

Y.H.Guo ^{[22
]}

Z.Guo ^{[8
]}

R.W.Hackenburg ^{[4
]}

S.Hans ^{[4
,23
]}

M.He ^{[6
]}

K.M.Heeger ^{[3
]}

Y.K.Heng ^{[6
]}

A.Higuera ^{[24
]}

Y.K.Hor ^{[25
]}

Y.B.Hsiung ^{[5
]}

B.Z.Hu ^{[5
]}

J.R.Hu ^{[6
]}

T.Hu ^{[6
]}

Z.J.Hu ^{[25
]}

H.X.Huang ^{[26
]}

X.T.Huang ^{[27
]}

机构：

[1] Institute of Modern Physics,East China University of Science and Technology

[2] University of Wisconsin

[3] Wright Laboratory and Department of Physics,Yale University

[4] Brookhaven National Laboratory

[5] Department of Physics,National Taiwan University

[6] Institute of High Energy Physics

[7] National United University

[8] Department of Engineering Physics,Tsinghua University

[9] Shenzhen University

[10] Sun Yat-Sen (Zhongshan) University

[11] North China Electric Power University

[12] Chinese University of Hong Kong

[13] Siena College,Loudonville

[14] Department of Physics and Astronomy,University of California

[15] University of Science and Technology of China

[16] Charles University,Faculty of Mathematics and Physics

[17] Department of Physics,University of Illinois at Urbana-Champaign

[18] Lawrence Berkeley National Laboratory

[19] Department of Physics,Illinois Institute of Technology

[20] Joint Institute for Nuclear Research

[21] Beijing Normal University

[22] Department of Nuclear Science and Technology,School of Energy and Power Engineering,Xi'an Jiaotong University

[23] Department of Chemistry and Chemical Technology,Bronx Community College

[24] Department of Physics,University of Houston

[25] Sun Yat-Sen Zhongshan University

[26] China Institute of Atomic Energy

[27] Shandong University

[28] Guangxi University

[29] Center for Neutrino Physics,Virginia Tech

[30] Institute of Physics,National Chiao-Tung University

[31] Department of Physics,University of Cincinnati

[32] Department of Physics,College of Science and Technology,Temple University

[33] Dongguan University of Technology

[34] Department of Physics,University of California

[35] Department of Physics,The University of Hong Kong

[36] School of Physics,Nankai University

[37] Department of Physics and Astronomy,Shanghai Jiao Tong University,Shanghai Laboratory for Particle Physics and Cosmology

[38] Joseph Henry Laboratories,Princeton University

[39] California Institute of Technology

[40] College of William and Mary

[41] Nanjing University

[42] China General Nuclear Power Group

[43] College of Electronic Science and Engineering,National University of Defense Technology

[44] Iowa State University

[45] Chongqing University

来源：

Chinese Physics C | 2021年 / 45卷 / 05期

基金：

中国国家自然科学基金; 美国国家科学基金会;

关键词：

D O I：

暂无

中图分类号：

O572.321 [];

学科分类号：

070202 ;

摘要：

The establishment of 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 was performed for electron-antineutrino signals that coincided with detected GW events,including GW150914,GW151012,GW151226,GW170104,GW170608,GW170814,and GW170817.We used three time windows of ±10,±500,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 were consistent with the expected background rates for all the three time windows.Assuming monochromatic spectra,we found upper limits（90%confidence level） of the 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.

引用

页码：194 / 205

页数：12

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