Published January 1, 2018 | Version v1
Journal article

Seasonal variation of the underground cosmic muon flux observed at Daya Bay

  • 1. Institute of Modern Physics, East China University of Science and Technology, Shanghai (China)
  • 2. University of Wisconsin, Madison, Wisconsin 53706 (United States)
  • 3. Wright Laboratory and Department of Physics, Yale University, New Haven, Connecticut 06520 (United States)
  • 4. Brookhaven National Laboratory, Upton, New York 11973 (United States)
  • 5. Department of Physics, National Taiwan University, Taipei (China)
  • 6. Nanjing University, Nanjing (China)
  • 7. Institute of High Energy Physics, Beijing (China)
  • 8. Chinese University of Hong Kong (Hong Kong)
  • 9. National United University, Miao-Li (China)
  • 10. Shandong University, Jinan (China)
  • 11. Department of Engineering Physics, Tsinghua University, Beijing (China)
  • 12. North China Electric Power University, Beijing (China)
  • 13. Shenzhen University, Shenzhen (China)
  • 14. Sun Yat-Sen (Zhongshan) University, Guangzhou (China)

Description

The Daya Bay Experiment consists of eight identically designed detectors located in three underground experimental halls named as EH1, EH2, EH3, with 250, 265 and 860 meters of water equivalent vertical overburden, respectively. Cosmic muon events have been recorded over a two-year period. The underground muon rate is observed to be positively correlated with the effective atmospheric temperature and to follow a seasonal modulation pattern. The correlation coefficient α, describing how a variation in the muon rate relates to a variation in the effective atmospheric temperature, is found to be αEH1 = 0.362±0.031, αEH2 = 0.433±0.038 and αEH3 = 0.641±0.057 for each experimental hall.

Availability note (English)

Available from http://dx.doi.org/10.1088/1475-7516/2018/01/001

Additional details

Publishing Information

Journal Title
Journal of Cosmology and Astroparticle Physics
Journal Volume
2018
Journal Issue
01
Journal Page Range
p. 001
ISSN
1475-7516