Muon flux measurement at China Jinping Underground Laboratory

被引:26
|
作者
Guo, Zi-yi [1 ,2 ]
Bathe-Peters, Lars [1 ,4 ]
Chen, Shao-min [1 ,2 ,3 ]
Chouaki, Mourad [1 ,5 ]
Dou, Wei [1 ,2 ]
Guo, Lei [1 ,2 ]
Hussain, Ghulam [1 ,2 ]
Li, Jin-jing [1 ,2 ]
Liu, Qian [6 ]
Luo, Guang [7 ]
Luo, Wen-tai [6 ]
Qi, Ming [8 ]
Shao, Wen-hui [1 ,2 ]
Tang, Jian [7 ]
Wan, Lin-yan [1 ,2 ]
Wang, Zhe [1 ,2 ,3 ]
Xu, Ben-da [1 ,2 ,3 ]
Xu, Tong [1 ,2 ]
Xu, Wei-ran [1 ,2 ]
Yang, Yu-zi [1 ,2 ]
Yeh, Minfang [9 ]
Zhao, Lin [1 ,2 ]
机构
[1] Tsinghua Univ, Dept Engn Phys, Beijing 100084, Peoples R China
[2] Tsinghua Univ, Ctr High Energy Phys, Beijing 100084, Peoples R China
[3] Tsinghua Univ, Minist Educ, Key Lab Particle & Radiat Imaging, Beijing, Peoples R China
[4] Tech Univ Berlin, Inst Phys, D-10623 Berlin, Germany
[5] Ecole Polytech Fed Lausanne, CH-1015 Lausanne, Switzerland
[6] Univ Chinese Acad Sci, Sch Phys Sci, Beijing 100049, Peoples R China
[7] Sun Yat Sen Univ, Sch Phys, Guangzhou 510275, Peoples R China
[8] Nanjing Univ, Sch Phys, Nanjing 210093, Peoples R China
[9] Brookhaven Natl Lab, Upton, NY 11973 USA
基金
美国能源部; 中国国家自然科学基金;
关键词
CJPL; cosmic-ray muon flux; angular distribution; neutrino detector; liquid scintillator;
D O I
10.1088/1674-1137/abccae
中图分类号
O57 [原子核物理学、高能物理学];
学科分类号
070202 ;
摘要
China Jinping Underground Laboratory (CJPL) is ideal for studying solar, geo-, and supernova neutrinos. A precise measurement of the cosmic-ray background is essential in proceeding with R&D research for these MeV-scale neutrino experiments. Using a 1-ton prototype detector for the Jinping Neutrino Experiment (JNE), we detected 264 high-energy muon events from a 645.2-day dataset from the first phase of CJPL (CJPL-I), reconstructed their directions, and measured the cosmic-ray muon flux to be (3.53 +/- 0.22(stat.) +/- 0.07(sys.)) x 10(-10) cm(-2)s(-1). The observed angular distributions indicate the leakage of cosmic-ray muon background and agree with simulation data accounting for Jinping mountain's terrain. A survey of muon fluxes at different laboratory locations, considering both those situated under mountains and those down mine shafts, indicates that the flux at the former is generally a factor of (4 +/- 2) larger than at the latter, with the same vertical overburden. This study provides a convenient back-of-the-envelope estimation for the muon flux of an underground experiment.
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页数:9
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