COSMIC RAY ACCELERATION AT PERPENDICULAR SHOCKS IN SUPERNOVA REMNANTS

Supernova remnants (SNRs) are believed to accelerate particles up to high energies through the mechanism of diffusive shock acceleration (DSA). Except for direct plasma simulations, all modeling efforts must rely on a given form of the diffusion coefficient, a key parameter that embodies the interac...

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Veröffentlicht in:	The Astrophysical journal 2014-09, Vol.792 (2), p.1-13
Hauptverfasser:	Ferrand, Gilles, Danos, Rebecca J, Shalchi, Andreas, Safi-Harb, Samar, Edmon, Paul, MENDYGRAL, PETER
Format:	Artikel
Sprache:	eng
Schlagworte:	ACCELERATION Alpha rays ASTROPHYSICS, COSMOLOGY AND ASTRONOMY CHARGED PARTICLES Coefficients Computer simulation COMPUTERIZED SIMULATION COSMIC RADIATION DIFFUSION DISTRIBUTION GALAXIES INJECTION INTERACTIONS Mathematical models MODIFICATIONS NONLINEAR PROBLEMS PLASMA SIMULATION SPECTRA SUPERNOVA REMNANTS TIME DEPENDENCE TURBULENCE
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