Detectors for high-energy messengers from the Universe

Abstract

High-energy messengers from the Universe comprise charged cosmic rays, gamma rays and neutrinos. Here we summarise the detection principles and detection schemes for these particles, with a focus on ground-based instruments which employ natural media such as air, ice, or water as their detection medium.

arXiv comment17 pages, 11 figures

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Cited by in corpus (4)

• CRPropa 3.2 -- an advanced framework for high-energy particle propagation in extragalactic and galactic spaces
• The Estimation of Fundamental Physics Parameters for Fermi-LAT Blazars
• High-Energy Galactic Cosmic Rays (Astro2020 Science White Paper)
• Multi-messenger astronomy with very-high-energy gamma-ray observations