Identifying Nearby UHECR Accelerators using UHE (and VHE) Photons
arXiv:0904.3903 · doi:10.1103/PhysRevLett.103.051102
Abstract
Ultra-high energy photons (UHE, E > 10^19 eV) are inevitably produced during the propagation of 10^20 eV protons in extragalactic space. Their short interaction lengths (<20 Mpc) at these energies, combined with the impressive sensitivity of the Pierre Auger Observatory detector to these particles, makes them an ideal probe of nearby ultra-high-energy cosmic ray (UHECR) sources. We here discuss the particular case of photons from a single nearby (within 30 Mpc) source in light of the possibility that such an object might be responsible for several of the UHECR events published by the Auger collaboration. We demonstrate that the photon signal accompanying a cluster of a few > 6x10^19 eV UHECRs from such a source should be detectable by Auger in the near future. The detection of these photons would also be a signature of a light composition of the UHECRs from the nearby source.
4 pages, 2 figures, accepted for publication in PRL
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Cited by in corpus (11)
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- Extragalactic propagation of ultrahigh energy cosmic-rays
- The Astrophysical Multimessenger Observatory Network (AMON): Performance and Science Program
- UHECR Composition Models
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- Selected Topics in Cosmic Ray Physics
- Tracing Cosmic accelerators with Decaying Neutrons
- Simulation study of GZK photon fluxes
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