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Separating beam-induced and cosmogenic muon backgrounds in the ICARUS detector

Conference ·
DOI:https://doi.org/10.2172/1997512· OSTI ID:1997512

Due to high cosmic ray flux near the earth's surface, the rejection of cosmogenic muon backgrounds is a preeminent concern for particle detectors using Liquid Argon Time Projection Chamber (LArTPC) technology. One such detector, ICARUS of the short baseline neutrino experiment, also observes muons generated from neutrino interactions with nuclei in the surrounding rock. Our analysis exploits the differences between cosmogenic and rock-generated muons to separate rock-generated muons from the background. We develop a selection with 96.5\% efficiency and 81\% accuracy. Use of this selection on data and Monte-Carlo indicates monte-carlo may underestimate the true rock muon flux. These results have implications for calibration of the ICARUS detector and tuning of simulation.

Research Organization:
Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States)
Sponsoring Organization:
USDOE Office of Science (SC), High Energy Physics (HEP) (SC-25)
DOE Contract Number:
AC02-07CH11359
OSTI ID:
1997512
Report Number(s):
FERMILAB-POSTER-23-195-STUDENT; oai:inspirehep.net:2685040
Country of Publication:
United States
Language:
English

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