Comments on the origin of cosmic rays

Details Comments on the origin of cosmic rays Comments on the origin of cosmic rays

Sep 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982izssr..46.1650g&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Samarkand, Uzbek SSR, Oct. 27-29, 1981.) Akademiia Nauk SSSR, Izvestiia, Ser

Physics

Antiprotons, Cosmic Rays, Particle Flux Density, Protons

Scientific paper

The origin of the relatively large flux of antiprotons observed in cosmic rays is discussed. It is suggested that the most probable explanation for the occurrence of this large flux is the presence of thick sources (20-100 g/sq cm) with a high proton-generating capacity; the nucleus of the Galaxy in its active stage might be such a source. A method is proposed for estimating the contribution of local sources to the concentration of cosmic rays observed at the earth.

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