Ultra-High Energy Cosmic Rays and Diffuse Photon Spectrum

Abstract

It is argued that if extragalactic magnetic fields are smaller than 2x10-12 G the flux of ultra-high energy photons of (a few)x10-1 eV cm-2s-1sr-1 predicted in the top-down models of UHE CR implies similar flux of the diffuse photons in the energy range 1015-1017 eV, which is close to the existing experimental limit.

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