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Ultra-High Energy Cosmic Rays: A Probe of Physics and Astrophysics at Extreme Energies

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arxiv astro-ph/0104291 v1 pith:DH7V4GZO submitted 2001-04-17 astro-ph hep-ph

classification astro-phhep-ph
keywords astrophysicscosmicenergiesphysicsraysenergyoriginprobe
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The origin of cosmic rays is one of the major unresolved questions in astrophysics. In particular, the highest energy cosmic rays observed possess macroscopic energies and their origin is likely associated with the most energetic processes in the Universe. They thus provide a probe of physics and astrophysics at energies that are unreached in laboratory experiments. Theoretical explanations range from acceleration of charged particles in astrophysical environments to particle physics beyond the well established Standard Model, and processes taking place at the earliest moments of our Universe. Distinguishing between these scenarios requires detectors with effective areas in the 1000 km^2 range which are now under construction or in the planning stage. Close connections with gamma-ray and neutrino astrophysics add to the interdisciplinary character of this field.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Evidence for the Sombrero Galaxy as an Accelerator of the Highest-Energy Cosmic Rays

    astro-ph.HE 2024-12 conditional novelty 6.0 of 10

    A maximum-likelihood search of Pierre Auger data finds a 3.3 sigma (global) association between a cosmic-ray multiplet and the Sombrero Galaxy, supporting AGN jet and lobe acceleration of UHECRs.

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