Hydromagnetic turbulence amplification in the vicinity of shock waves and the maximum energies of accelerated particles in supernova remnants

Details Hydromagnetic turbulence amplification in the vicinity of shock waves and the maximum energies of accelerated particles in supernova remnants Hydromagnetic turbulence amplification in the vicinity of shock waves and the maximum energies of accelerated particles in supernova remnants

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.

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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.

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