Acceleration of charged particles in the shell of a supernova

Details Acceleration of charged particles in the shell of a supernova Acceleration of charged particles in the shell of a supernova

Dec 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979izyer..43.2480k&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Yerevan, Armenian SSR, June 1979.) Akademiia Nauk SSSR, Izvestiia, Seriia Fi

Physics

Charged Particles, Cosmic Rays, Particle Acceleration, Stellar Envelopes, Supernovae, Energetic Particles, Energy Spectra, Galactic Radiation, Shock Wave Propagation, Stellar Evolution

Scientific paper

Supernovae are considered as a possible source of galactic cosmic rays. The energy spectrum characteristics of protons and electrons accelerated by the regular mechanism (i.e., on shock waves) in supernova shells are examined. Shell evolution is discussed in relation to cosmic ray generation, and the energy contribution of supernovae to cosmic rays is examined.

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