Ultra-High Energy Cosmic Rays: Past, Present and Future
A special issue of Universe (ISSN 2218-1997). This special issue belongs to the section "Space Science".
Deadline for manuscript submissions: 31 October 2025 | Viewed by 45

Special Issue Editors
Interests: very-high energy astrophysics; detectors; artificial intelligence
Special Issues, Collections and Topics in MDPI journals
Special Issue Information
Dear Colleagues,
Cosmic rays, one of the main pillars of modern astrophysics, convey valuable information about distant energetic objects and phenomena in the universe. These charged particles range from electrons and protons to iron nuclei, with their energies extending across eleven orders of magnitude. The propagation of these particles through magnetic fields scatters their initial trajectories such that, by the time they reach Earth, their original sources become obscured.
Upon entering Earth’s atmosphere, cosmic rays with energies exceeding approximately 1 GeV (10⁹ eV) initiate extensive cascades of secondary particles and radiation. These cascades can be observed using various distributed detection systems, whose scale and complexity vary significantly depending on the energy’s range of interest.
Modern observatories now reach energies of 1 EeV (1018 eV) and beyond, with technological studies entering an era of ultra-high-energy cosmic-ray (UHECR) research and revealing the extragalactic origin of these particles. Decades of UHECR observations have revealed their properties and their connections with uncharged messengers: neutrinos and gamma rays.
In this Special Issue, we welcome the submission of articles that review key historical results, highlight advances in the field of multi-messenger astronomy, and discuss future projects.
Dr. Dmitriy Kostunin
Dr. Vladimir Lenok
Guest Editors
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Keywords
- ultra-high energy cosmic rays
- astrophysical neutrino
- high-energy gamma rays
- multimessenger astronomy
- cosmic accelerators
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