Influence of the universal microwave background radiation on the extragalactic cosmic-ray spectrum

Details Influence of the universal microwave background radiation on the extragalactic cosmic-ray spectrum Influence of the universal microwave background radiation on the extragalactic cosmic-ray spectrum

Aug 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994phrvd..50.1892a&link_type=abstract

Physical Review D (Particles and Fields), Volume 50, Issue 3, 1 August 1994, pp.1892-1900

Physics

74

Cosmic Rays, Background Radiations

Scientific paper

Features of the spectrum of the most energetic cosmic-ray protons produced by their passage through the 2.7 K universal background radiation are investigated by Monte Carlo techniques. We discuss the influence of various factors on the spectrum of protons observed at Earth with energies above 3×1019 eV. These factors include the shape of the initial cosmic-ray spectrum, the spatial distribution of sources, and the energy-dependent diffusion and escape of particles from a confinement region.

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