Author:
Guo Zi-yi,Bathe-Peters Lars,Chen Shao-min,Chouaki Mourad,Dou Wei,Guo Lei,Hussain Ghulam,Li Jin-jing,Liu Qian,Luo Guang,Luo Wen-tai,Qi Ming,Shao Wen-hui,Tang Jian,Wan Lin-yan,Wang Zhe,Xu Ben-da,Xu Tong,Xu Wei-ran,Yang Yu-zi,Yeh Minfang,Zhao Lin
Abstract
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.
Subject
Astronomy and Astrophysics,Instrumentation,Nuclear and High Energy Physics
Cited by
27 articles.
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