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Published on: April 17, 2018
Simple coincidence technique for cosmic-ray intensity exploration via low-energy photon detection
J Knezevic1, D Mrdja1, K Bikit1
1University of Novi Sad, Faculty of Sciences, Department of Physics, Trg Dositeja Obradovica 3, 21000, Novi Sad, Serbia.
Cosmic-ray intensity affects rare event searches by altering detector backgrounds. This study uses low-energy photon spectra to monitor cosmic-ray-induced particle cascades near Earth
Area of Science:
- Nuclear physics
- Astroparticle physics
- Cosmic-ray physics
Background:
- Cosmic-ray intensity fluctuations impact sensitive physics experiments by changing detector background rates.
- Understanding these variations is crucial for distinguishing rare signals from background noise.
Purpose of the Study:
- To develop and validate a method for monitoring cosmic-ray intensity using low-energy photon background spectra.
- To investigate the production of secondary particles induced by cosmic rays at the Earth's surface.
Main Methods:
- Utilized a coincidence system with a plastic scintillator and an extended-range High-Purity Germanium (HPGe) detector.
- Acquired low-energy photon spectra and employed the GEANT4 toolkit for system simulation.
- Compared simulated and experimental spectral data.
Main Results:
- Established a method to analyze cosmic-ray-induced photon spectra.
- Validated the experimental setup through comparison with GEANT4 simulations.
- Identified potential for monitoring cosmic-ray intensity variations.
Conclusions:
- Low-energy photon background spectra serve as a viable tool for cosmic-ray intensity monitoring.
- The developed methodology aids in characterizing detector backgrounds for rare event searches.
- Further analysis can explore periodic behaviors in photon emission related to cosmic rays.
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