Imaging via Cosmic Muon Induced Secondaries

  • Gergő Hamar HUN-REN Wigner Research Centre for Physics, Budapest, Hungary https://orcid.org/0000-0002-2268-7830
  • Kristina Demirhan University of Novi Sad, Faculty of Sciences, Department of Physics, Novi Sad, Serbia
  • Dániel Hajnal HUN-REN Wigner Research Centre for Physics, Budapest, Hungary
  • Dusan Mrdja University of Novi Sad, Faculty of Sciences, Department of Physics, Novi Sad, Serbia
  • Gábor Galgóczi HUN-REN Wigner Research Centre for Physics, Budapest, Hungary
  • Dezső Varga HUN-REN Wigner Research Centre for Physics, Budapest, Hungary
Keywords: muography, material identification, gaseous detectors

Abstract

As cosmic muons traverse a target, they interact with it, producing secondary radiation, whose spectrum
depends on the material-composition of the target. This imaging technique is sensitive to low-Z materials
as well, opening a novel noninvasive material-identification method for medium-sized obscure targets.
Our Hungarian-Serbian collaboration pioneered in demonstrating experimentally this unique method, using
gaseous trackers for the muons and a scintillator array and germanium detector for the secondaries.
Results have proven imaging possibilities ranging from metals to soft-tissue targets. Corresponding Geant4
simulations have revealed forward-sideward asymmetry and sensitivity to the electron/gamma ratio. The
former is materialized in a new experimental setup, with large coverage via segmented scintillator arrays,
and a combined and compact DAQ, with an electron-tagging possibility. The paper describes the recent
results in imaging via secondaries and details the new enhanced experimental setup and its first results.

Published
2024-05-10
How to Cite
[1]
G. Hamar, K. Demirhan, D. Hajnal, D. Mrdja, G. Galgóczi, and D. Varga, “Imaging via Cosmic Muon Induced Secondaries”, Journal of Advanced Instrumentation in Science, vol. 2024, no. 1, May 2024.
Section
International Workshop on Cosmic-Ray Muography (Muography2023), Naples, Italy