Particle Acceleration in Kinetic Plasma Processes

Physics – Plasma Physics

Scientific paper

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Scientific paper

The acceleration of high energy particles in astrophysical sources has attracted our attention for a long time, and their origins remain a central problem in astroplasma physics. We review recent progress that was made to understand both the dynamic structure of the source region and the connection with particle acceleration, and specifically discuss that not only the stochastic acceleration such as the first order Fermi acceleration, but also the direct acceleration seen in the shock front or in the reconnection region can contribute to the origins of the astrophysical nonthermal particles.

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