Astrophysical implications of cosmic-ray antiprotons

Details Astrophysical implications of cosmic-ray antiprotons Astrophysical implications of cosmic-ray antiprotons

Sep 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974phrvd..10.1731g&link_type=abstract

Physical Review D, vol. 10, Issue 6, pp. 1731-1735

Physics

31

Scientific paper

The production and propagation of secondary cosmic-ray antiprotons is discussed. The flux expected on the basis of the usual picture of cosmic-ray propagation, including an energy-dependent confinement time, is calculated. It is also pointed out that kinematical features of the expected secondary-antiproton spectrum provide a possible way to discriminate between secondary antiprotons and a hypothetical primary p¯ component in the cosmic radiation.

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