Generation of cosmic rays by supernovae in the inhomogeneous interstellar medium

Details Generation of cosmic rays by supernovae in the inhomogeneous interstellar medium Generation of cosmic rays by supernovae in the inhomogeneous interstellar medium

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988izssr..52.2290b&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Alma-Ata, Kazakh SSR, Sept. 13-15, 1988) Akademiia Nauk SSSR, Izvestiia, Ser

Computer Science

1

Aerospace Environments, Galactic Cosmic Rays, Intergalactic Media, Milky Way Galaxy, Supernovae, Chemical Composition, Dynamic Characteristics, Relativistic Electron Beams, Stellar Spectra

Scientific paper

The production of secondary antiprotons in young supernova shells with
an internal pulsar source of cosmic rays is calculated. The observed
antiproton/proton ratio can be explained by assuming that these sources
produce 15-25 percent of all galactic cosmic rays.

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