PoS - Proceedings of Science
Volume 395 - 37th International Cosmic Ray Conference (ICRC2021) - CRI - Cosmic Ray Indirect
Muography background sources: simulation, characterization, and machine-learning rejection
J. Peña Rodríguez*, R. de'León-Barrios, A. Ramírez-Muñóz, D. Villabona-Ardila, M. Suárez-Durán, A. Vásquez-Ramírez, H. Asorey and L.A. Núñez
Full text: pdf
Pre-published on: August 01, 2021
Published on: March 18, 2022
Muography scans large-size objects, natural or anthropic, by recording the atmospheric muon flux crossing them. The traversing muon flux, four orders of magnitude lower than the vertical muon flux, suffers an overwhelming background. The background sources are scattered muons, electromagnetic particles, reverse trajectory particles, and particles arriving simultaneously. We carried out Monte Carlo simulations to characterize such background sources. We estimated the scattered muon energy-angular spectrum and the cosmic ray components impinging the Muon Telescope --MuTe. We quantified the muography background using the Time-of-Flight and Water Cherenkov detector measurements of MuTe. We explored machine learning techniques to reject the background events.
DOI: https://doi.org/10.22323/1.395.0400
How to cite

Metadata are provided both in "article" format (very similar to INSPIRE) as this helps creating very compact bibliographies which can be beneficial to authors and readers, and in "proceeding" format which is more detailed and complete.

Open Access
Creative Commons LicenseCopyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.