Statistics – Computation
Scientific paper
Aug 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988azh....65..763f&link_type=abstract
Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 65, July-Aug. 1988, p. 763-770. In Russian.
Statistics
Computation
1
Magnetohydrodynamic Turbulence, Particle Acceleration, Shock Wave Propagation, Supernova Remnants, Computational Astrophysics, Particle Energy, Self Consistent Fields
Scientific paper
The authors consider a self-consistent mechanism of diffusive shock acceleration with particles generating the MHD waves. They calculate spectral and spatial characteristics of the turbulence, diffusion coefficient and the particle distribution function. From a comparison of the characteristic particle acceleration time with supernova remnants lifetimes they determine the particle limiting energies, which can be achieved within the context of the considered mechanism, Emax ≡ 102 - 103GeV.
Fedorenko V. N.
Flejshman G. D.
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