Cosmic ray antiprotons in closed galaxy model

Details Cosmic ray antiprotons in closed galaxy model Cosmic ray antiprotons in closed galaxy model

Jun 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981stin...8129061p&link_type=abstract

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Astronomy and Astrophysics

Astronomy

Abundance, Antiprotons, Astronomical Models, Cosmic Rays, Galaxies, Particle Flux Density, Galactic Nuclei, Interstellar Matter, Particle Acceleration

Scientific paper

The flux of secondary antiprotons expected for the leaky-box model was calculated as well as that for the closed galaxy model of Peters and Westergard (1977). The antiproton/proton ratio observed at several GeV is a factor of 4 higher than the prediction for the leaky-box model but is consistent with that predicted for the closed galaxy model. New low energy data is not consistent with either model. The possibility of a primary antiproton component is discussed.

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