White Paper on Ultra-High Energy Cosmic Rays
A. V. Olinto, J. H. Adams, C. D. Dermer, J. F. Krizmanic, J. W., Mitchell, P. Sommers, T. Stanev, F. W. Stecker, Y. Takahashi

TL;DR
This paper discusses the importance of identifying the origins of ultra-high energy cosmic rays, the potential sources, and how upcoming observatories can advance our understanding of the universe's most energetic phenomena.
Contribution
It highlights the scientific goals, challenges, and technological advancements needed for next-generation observatories to study ultra-high energy cosmic rays.
Findings
Sources of the highest energy cosmic rays remain unknown.
Next-generation observatories will significantly increase exposure and sensitivity.
Studying these cosmic rays will reveal insights into astrophysical environments and fundamental physics.
Abstract
A fundamental question that can be answered in the next decade is: WHAT IS THE ORIGIN OF THE HIGHEST ENERGY COSMIC PARTICLES? The discovery of the sources of the highest energy cosmic rays will reveal the workings of the most energetic astrophysical environments in the recent universe. Candidate sources range from the birth of compact objects to explosions related to gamma-ray bursts or generated around supermassive black holes in active galactic nuclei. In addition to beginning a new era of high-energy astrophysics, the study of ultra-high energy cosmic rays will constrain the structure of the Galactic and extragalactic magnetic fields. The propagation of these particles from source to Earth also probes the cosmic background radiation and gives insight into particle interactions at orders of magnitude higher energy than can be achieved in terrestrial laboratories. Next generation…
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Dark Matter and Cosmic Phenomena · Gamma-ray bursts and supernovae
