Derivation of antiproton-proton flux ratio from the closed galaxy model

Details Derivation of antiproton-proton flux ratio from the closed galaxy model Derivation of antiproton-proton flux ratio from the closed galaxy model

Jul 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.146..151p&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 146, no. 1, July 1988, p. 151-156.

Statistics

Computation

1

Antiprotons, Astronomical Models, Computational Astrophysics, Galaxies, Particle Flux Density, Protons, Cosmic Rays, Proton-Proton Reactions

Scientific paper

The antiproton-proton flux ratio has been estimated from the closed galaxy model of Peters and Westergaard (1977) by using the latest primary nucleon spectrum and pp - p(-)X inclusive reaction accelerator results. The derived p(-)/p flux ratio is about three times higher than those expected from the leaky box model. The results have been compared with the previous estimates by different authors.

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