Production of secondary particles in molecular clouds

Details Production of secondary particles in molecular clouds Production of secondary particles in molecular clouds

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988izssr..52.2312d&link_type=abstract

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

Physics

Gamma Rays, Molecular Clouds, Particle Interactions, Secondary Cosmic Rays, Particle Acceleration, Satellite Observation

Scientific paper

Gamma radiation and secondary-particle production in molecular clouds are investigated theoretically, assuming that the statistical particle acceleration mechanism proposed by Gurevich et al. (1985) operates in these clouds. The stationary spectrum of cosmic rays in these clouds is calculated, and the production rate of secondary particles (pions, muons, electrons, positrons, and antiprotons) is determined.

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