Ultra High Energy Cosmic Rays: The theoretical challenge
arXiv:astro-ph/0002006 · doi:10.1016/S0370-1573(00)00028-4
Abstract
The origin of the highest-energy cosmic rays remains a mystery. The lack of a high energy cutoff in the cosmic ray spectrum together with an apparently isotropic distribution of arrival directions have strongly constrained most models proposed for the generation of these particles. An overview of the present state of theoretical proposals is presented. Astrophysical accelerators as well as top-down scenarios are reviewed along with their most general signatures. The origin and nature of these ultra-high energy particles will be tested by future observations and may indicate as well as constrain physics beyond the standard model of particle physics.
25 page review, 5 figs, to be published in the David Schramm Memorial Volume of Physics Reports, latex file; elsart
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Cited by in corpus (68)
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- Neutrinos from propagation of ultra-high energy protons
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- Neutrino Detection with Inclined Air Showers
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- Cosmic Neutrinos and New Physics beyond the Electroweak Scale
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- UHECR propagation in the Galaxy: clustering versus isotropy
- Determination of the calorimetric energy in extensive air showers
- Absolute Neutrino Mass Determination
- In Search for Extraterrestrial High Energy Neutrinos
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- Cosmic Rays and the Search for a Lorentz Invariance Violation
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- Ultra-High Energy Cosmic Ray Nuclei from Individual Magnetized Sources
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- Gravitational diffraction radiation
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- Seeking for the observational manifestation of de Sitter Relativity
- The Future of Ultra High Energy Cosmic Rays
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