High-Energy Galactic Cosmic Rays (Astro2020 Science White Paper)
arXiv:1903.07713
Abstract
The origin of the highest energy Galactic cosmic rays is still not understood, nor is the transition to EeV extragalactic particles. Scientific progress requires enhancements of existing air-shower arrays, such as: IceCube with its surface detector IceTop, and the low-energy extensions of both the Telescope Array and the Pierre Auger Observatory.
Science White Paper for the Astronomy and Astrophysics Decadal Survey (Astro2020)
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Cited by in corpus (5)
- Ultra-High-Energy Cosmic Rays: The Intersection of the Cosmic and Energy Frontiers
- Phenomenological Effects of CPT and Lorentz Invariance Violation in Particle and Astroparticle Physics
- The cosmic-ray spectrum in the PeV to EeV energy range
- Design and Expected Performance of the IceCube-Gen2 Surface Array and its Radio Component (ARENA2022)
- News from Cosmic Ray Air Showers (ICRC 2019 -- Cosmic Ray Indirect Rapport)