Theoretical predictions for cosmic ray secondary antiprotons

Details Theoretical predictions for cosmic ray secondary antiprotons Theoretical predictions for cosmic ray secondary antiprotons

May 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997adspr..19..775g&link_type=abstract

Advances in Space Research, Volume 19, Issue 5, p. 775-780.

Physics

Scientific paper

We calculate the flux of secondary antiprotons produced by cosmic rays during propagation in the interstellar medium. We illustrate with several examples how the resulting antiproton to proton ratio as measured depends on the assumed primary spectrum and on propagation. We give particular attention to the kinematic suppression of secondary antiprotons below 1 GeV, which is a signature of secondary production.

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