Particle acceleration up to 10 exp 20 eV

Details Particle acceleration up to 10 exp 20 eV Particle acceleration up to 10 exp 20 eV

Aug 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992aipc..264..400i&link_type=abstract

In: Particle acceleration in cosmic plasmas; Proceedings of the Workshop, Bartol Research Inst., Newark, DE, Dec. 4-6, 1991 (A93

Mathematics

Probability

8

Energy Spectra, Galactic Cosmic Rays, Particle Acceleration, Particle Interactions, Supernova Remnants, Charged Particles, Frequency Distribution, Probability Distribution Functions

Scientific paper

A scenario for second-stage acceleration of the Galactic cosmic rays beyond 10 exp 14 eV via multiple interaction with SNRs in the Galactic disc is investigated. A numerical scheme taking into consideration the size frequency distribution of SNRs, the probability distribution of energy gain/loss during SNR encounter and the compositional abundances of the cosmic ray nuclei is used to illustrate the quantitative aspects of such process.

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