Non-variable cosmologically distant gamma-ray emitters as a propagation imprint of ultra-high-energy protons

Astronomy and Astrophysics

Volumn 536, Issue , 2011, Pages

  Prosekin, A Yu ^a   Kelner, S R ^a   Aharonian, F A ^a,b  

^a MAX PLANCK INSTITUT FÜR KERNPHYSIK   (Germany)

^b DUBLIN INSTITUTE FOR ADVANCED STUDIES   (Ireland)

Author keywords

Astroparticle physics; Gamma rays: general; Magnetic fields; X rays: general

Indexed keywords

ASTROPARTICLE PHYSICS; CHANDRA; COSMIC MICROWAVE BACKGROUND RADIATION; DETECTABILITY; ENERGY BUDGETS; ENERGY TRANSFER EFFICIENCY; HIGH ENERGY GAMMA RAYS; RED SHIFT; SECONDARY ELECTRONS; SECONDARY PARTICLES; SPECTRAL DISTRIBUTION; X-RAY ENERGIES; X-RAYS: GENERAL;

COSMOLOGY; ENERGY CONVERSION; ENERGY DISSIPATION; HIGH ENERGY PHYSICS; MAGNETIC FIELDS; PROTONS; SYNCHROTRON RADIATION; SYNCHROTRONS;

GAMMA RAYS;

EID: 82955194918     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201117231     Document Type: Article

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