Energy spectrum of ultra high energy cosmic rays

Details Energy spectrum of ultra high energy cosmic rays Energy spectrum of ultra high energy cosmic rays

Nov 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975natur.258..217w&link_type=abstract

Nature, vol. 258, Nov. 20, 1975, p. 217, 218.

Astronomy and Astrophysics

Astronomy

5

Astronomical Models, Cosmic Rays, Energy Spectra, Energy Dissipation, Heavy Nuclei, Infrared Spectra, Spectrum Analysis

Scientific paper

The 'supercluster enhancement' model proposed by Strong et al. (1974) is considered, taking into account extragalactic protons. A graph is presented which shows the fractional rate of energy loss for the case where only the 2.7 K radiation is considered and its modification when the 'high' infrared spectrum is included. A rather smooth variation over the whole range is observed. The significance of these findings for the supercluster enhancement model is discussed.

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