The environmental monitoring system at the COSINE-100 experiment

H. Kim, G. Adhikari,E. Barbosa de Souza,N. Carlin, J. J. Choi,S. Choi,M. Djamal,A. C. Ezeribe, L. E. França,C. Ha,I. S. Hahn,E. J. Jeon,J. H. Jo,H. W. Joo, W. G. Kang,M. Kauer,H. J. Kim,K. W. Kim,S. H. Kim,S. K. Kim,W. K. Kim,Y. D. Kim,Y. H. Kim,Y. J. Ko,E. K. Lee,H. Lee,H. S. Lee,H. Y. Lee,I. S. Lee,J. Lee, J. Y. Lee,M. H. Lee,S. H. Lee,S. M. Lee,D. S. Leonard,B. B. Manzato,R. H. Maruyama, R. J. Neal,S. L. Olsen, B. J. Park,H. K. Park,H. S. Park,K. S. Park,R. L. C. Pitta,H. Prihtiadi,S. J. Ra,C. Rott, K. A. Shin,A. Scarff,N. J. C. Spooner,W. G. Thompson,L. Yang, G. H. Yu

JOURNAL OF INSTRUMENTATION（2022）

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摘要

The COSINE-100 experiment is designed to test the DAMA experiment which claimed an observation of a dark matter signal from an annual modulation in their residual event rate. To measure the 1 %-level signal amplitude, it is crucial to control and monitor nearly all environmental quantities that might systematically mimic the signal. The environmental monitoring also helps ensure a stable operation of the experiment. Here, we describe the design and performance of the centralized environmental monitoring system for the COSINE-100 experiment.

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关键词

Dark Matter detectors (WIMPs, axions, etc.), Gamma detectors (scintillators, CZT, HPGe, HgI etc), Very low-energy charged particle detectors

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