Particle acceleration in giant molecular clouds

Details Particle acceleration in giant molecular clouds Particle acceleration in giant molecular clouds

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984izyak..48.2070d&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Yakutsk, USSR, July 1984) Akademiia Nauk SSSR, Izvestiia, Seriia Fizicheskai

Computer Science

Cosmic Rays, Molecular Clouds, Particle Acceleration, Plasma-Particle Interactions, Electron Acceleration, Fermi Surfaces, Magnetic Flux, Plasma-Electromagnetic Interaction, Protons

Scientific paper

The paper examines the acceleration of cosmic rays by the Fermi II mechanism, formed by turbulence in giant molecular clouds. According to this mechanism, the interaction of the neutral and charged components in the clouds can lead to the excitation of random magnetic fields, which are responsible for the acceleration. The acceleration of electrons and protons in molecular clouds due to the Fermi II mechanism is examined. Stationary solutions are obtained for the transport equations.

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