Ultra-High-Energy Cosmic Rays from the Radio Lobes of AGNs
Sep, 20088 pages
Published in:
- Mon.Not.Roy.Astron.Soc. 391 (2008) 1100-1106
e-Print:
- 0809.3686 [astro-ph]
View in:
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Abstract: (arXiv)
In the past year, the HiRes and Auger collaborations have reported the discovery of a high-energy cutoff in the ultra-high energy cosmic-ray (UHECR) spectrum, and an apparent clustering of the highest energy events towards nearby active galactic nuclei (AGNs). Consensus is building that such -- eV particles are accelerated within the radio-bright lobes of these sources, but it is not yet clear how this actually happens. In this paper, we report (to our knowledge) the first treatment of stochastic particle acceleration in such environments from first principles, showing that energies eV are reached in years for protons. However, our findings reopen the question regarding whether the high-energy cutoff is due solely to propagation effects, or whether it does in fact represent the maximum energy permitted by the acceleration process itself.- cosmic rays
- physical data and processes: acceleration of particles
- plasmas
- turbulence galaxies: active
- nuclei
- cosmic radiation: UHE
- particle: acceleration
- magnetic field: turbulence
- time dependence
- cosmic radiation: energy spectrum
References(40)
Figures(7)