The injection and acceleration of particles in oblique shocks - A unified Monte Carlo description

Details The injection and acceleration of particles in oblique shocks - A unified Monte Carlo description The injection and acceleration of particles in oblique shocks - A unified Monte Carlo description

May 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993apj...409..327b&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 409, no. 1, p. 327-332.

Astronomy and Astrophysics

Astronomy

29

Mach Number, Monte Carlo Method, Oblique Shock Waves, Particle Acceleration, Shock Wave Interaction, Supernova Remnants, Cosmic Plasma, Magnetic Field Configurations, Radio Jets (Astronomy), Radio Observation

Scientific paper

Important problems are discussed concerning the effects of shock geometry on the injection of thermal particles and the process of standard Fermi particle acceleration in general. In pursuit of a self-consistent model that simultaneously describes shock structure and particle acceleration in shocks of arbitrary obliquity, a Monte Carlo simulation developed for parallel shocks is generalized to address oblique geometries. Attention is given to initial results concerning the ways in which injection and acceleration efficiency varies with obliquity and Mach number.

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