Ultra-High Energy Cosmic Rays and Diffuse Photon Spectrum

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dc.creatorTinyakov, P. G.
dc.date1999-09-14
dc.date.accessioned2026-07-07T02:33:16Z
dc.date.available2026-07-07T02:33:16Z
dc.descriptionIt 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.
dc.descriptionTalk given at XI Rencontres de Blois. 3 pages, no figures
dc.identifierhttps://arxiv.org/abs/astro-ph/9909244
dc.identifierhttp://arxiv.org/abs/astro-ph/9909244
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/14776
dc.subjectAstrophysics
dc.titleUltra-High Energy Cosmic Rays and Diffuse Photon Spectrum
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