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Ultra-High Energy Cosmic Rays and Diffuse Photon Spectrum

P. G. Tinyakov
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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^{-2}s^{-1}sr^{-1} predicted in the top-down models of UHE CR implies similar flux of the diffuse photons in the energy range 10^{15}-10^{17} eV, which is close to the existing experimental limit.

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P. G. Tinyakov. 1999-09-14. Ultra-High Energy Cosmic Rays and Diffuse Photon Spectrum. https://arxiv.org/abs/astro-ph/9909244

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