Explanations of the spectral shape in the energy range from 100 to 100,000,000 TeV

Details Explanations of the spectral shape in the energy range from 100 to 100,000,000 TeV Explanations of the spectral shape in the energy range from 100 to 100,000,000 TeV

Jan 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975rspta.277..429w&link_type=abstract

(Royal Society, Discussion on the Origin of the Cosmic Radiation, London, England, Feb. 20, 21, 1974.) Royal Society (London), P

Physics

Nuclear Physics

4

Astronomical Models, Energy Spectra, Interstellar Matter, Nuclei (Nuclear Physics), Primary Cosmic Rays, Spectrum Analysis, Black Body Radiation, Frequency Distribution, Gamma Rays, Magnetohydrodynamic Waves, Particle Diffusion, Pulsars, Spectral Line Width, Wave Interaction

Scientific paper

There is evidence suggesting an increase in slope of the energy spectrum of primary cosmic-ray nuclei at about 3000 TeV. Alternative explanations are advanced for this change, which are related to diffusion of particles of galactic origin or blackbody cutoff effects for particles of extragalactic origin. At higher energies there appear to be particles of energy up to 100,000,000 TeV. The evidence is examined critically, and alternative explanations are put forward for the spectral shape in this region.

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