Physics – Nuclear Physics
Scientific paper
Aug 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....2..354s&link_type=abstract
In its 19th Intern. Cosmic Ray Conf., Vol. 2 p 354-357 (SEE N85-34006 22-93)
Physics
Nuclear Physics
Antiprotons, Cosmic Rays, Energy Spectra, Baryons, Cosmology, Helium Ions, Intergalactic Media, Models, Nuclei (Nuclear Physics), Protons, Spectrum Analysis
Scientific paper
It may be possible to account for a previously puzzling feature - a bump in the energy range 10 to the 14th power eV to 10 to the 15th power - of the cosmic ray spectrum by hypothesizing a primary extragalactic origin for the bulk of the observed cosmic ray antiprotons, although such an explanation is not unique. In this model, most of the cosmic rays above 10 to the 15th power eV are extragalactic. A method is described of testing this hypothesis experimentally.
Stecker Floyd W.
Wolfendale Arnold W.
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