Calculation of cosmic ray antiproton-proton ratio

Details Calculation of cosmic ray antiproton-proton ratio Calculation of cosmic ray antiproton-proton ratio

Jan 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...252l..57g&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 252, Jan. 15, 1982, p. L57-L59. Research supported by the U.S. Depar

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10

Antiprotons, Cosmic Rays, Particle Interactions, Protons, Particle Flux Density, Secondary Cosmic Rays

Scientific paper

The conflicting results obtained by the independently conducted antiproton-to-proton ratio calculations of Gaisser and Maurer (1973) and Badhwar et al (1975) have obscured the interpretation of recent cosmic ray antiproton measurements. The apparent differences between the two calculations have been resolved upon detailed reexamination, showing that the Gaisser and Maurer calculation was essentially correct. It is demonstrated that the reported antiproton fluxes are higher than expected for secondary antiprotons in conventional models of cosmic ray propagation, as has been indicated by other recent calculations.

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