Muon flux measurement at China Jinping Underground Laboratory
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 Neutr...
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Published in | Chinese physics C Vol. 45; no. 2; p. 25001 |
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Main Authors | , , , , , , , , , , , , , , , , , , , , , |
Format | Journal Article |
Language | English |
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01.02.2021
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Abstract | 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
cm
s
. 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
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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AbstractList | 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 $(3.53\pm0.22_{\rm{stat.}}\pm0.07_{\rm{sys.}})\times10^{-10}$ 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 $(4\pm2)$ larger than at the latter, with the same vertical overburden. In conclusion, this study provides a convenient back-of-the-envelope estimation for the muon flux of an underground experiment. 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 cm s . 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 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. |
Author | Guo, Zi-yi Wang, Zhe Tang, Jian Xu, Tong Guo, Lei Luo, Wen-tai Zhao, Lin Qi, Ming Yang, Yu-zi Chouaki, Mourad Hussain, Ghulam Xu, Wei-ran Yeh, Minfang Luo, Guang Shao, Wen-hui Xu, Ben-da Liu, Qian Chen, Shao-min Li, Jin-jing Dou, Wei Wan, Lin-yan Bathe-Peters, Lars |
Author_xml | – sequence: 1 givenname: Zi-yi surname: Guo fullname: Guo, Zi-yi – sequence: 2 givenname: Lars surname: Bathe-Peters fullname: Bathe-Peters, Lars – sequence: 3 givenname: Shao-min surname: Chen fullname: Chen, Shao-min – sequence: 4 givenname: Mourad surname: Chouaki fullname: Chouaki, Mourad – sequence: 5 givenname: Wei surname: Dou fullname: Dou, Wei – sequence: 6 givenname: Lei surname: Guo fullname: Guo, Lei – sequence: 7 givenname: Ghulam surname: Hussain fullname: Hussain, Ghulam – sequence: 8 givenname: Jin-jing surname: Li fullname: Li, Jin-jing – sequence: 9 givenname: Qian surname: Liu fullname: Liu, Qian – sequence: 10 givenname: Guang surname: Luo fullname: Luo, Guang – sequence: 11 givenname: Wen-tai surname: Luo fullname: Luo, Wen-tai – sequence: 12 givenname: Ming surname: Qi fullname: Qi, Ming – sequence: 13 givenname: Wen-hui surname: Shao fullname: Shao, Wen-hui – sequence: 14 givenname: Jian surname: Tang fullname: Tang, Jian – sequence: 15 givenname: Lin-yan surname: Wan fullname: Wan, Lin-yan – sequence: 16 givenname: Zhe surname: Wang fullname: Wang, Zhe – sequence: 17 givenname: Ben-da surname: Xu fullname: Xu, Ben-da – sequence: 18 givenname: Tong surname: Xu fullname: Xu, Tong – sequence: 19 givenname: Wei-ran surname: Xu fullname: Xu, Wei-ran – sequence: 20 givenname: Yu-zi surname: Yang fullname: Yang, Yu-zi – sequence: 21 givenname: Minfang surname: Yeh fullname: Yeh, Minfang – sequence: 22 givenname: Lin surname: Zhao fullname: Zhao, Lin |
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Title | Muon flux measurement at China Jinping Underground Laboratory |
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