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Simulation study of GZK photon fluxes · Around

2009

Simulation study of GZK photon fluxes

Kuempel, Daniel, Kampert, Karl-Heinz, Risse, Markus

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The composition of ultra-high energy (UHE) cosmic rays E>10^17 eV is still unknown.

The observation of UHE photons would extend the observed electromagnetic spectrum to highest energy and open a new channel for multimessenger observations in the universe.
Current limits on the photon flux already constrain ``exotic'' scenarios where a large number of photons is expected by the decay products of supermassive X-particles.
Motivated by the growing exposure of UHE cosmic ray experiments - like the Pierre Auger Observatory - the observation of conventionally produced GZK photons may be in reach in the near future.

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Then

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Original
2008
Later among the works it cites.
D. Kuempel, K.-H. Kampert, M. Risse, Proc. 21 st European Cosmic Ray Symposium (ECRS), Košice Slowakia Sep. 2008, 6.21
2008
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I. V. Moskalenko, L. Stawarz, T. A. Porter and C. C. Cheung, Astrophys. J. 693
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