Relativistic Plasma Physics. 7. Relativistic Particle Acceleration as Origin of Cosmic Ray.
M. Hoshino
Abstract
Open-access reader
M. Hoshino
Abstract
Open-access reader
The origin of high energy particles seen radiating in astrophysical synchrotron sources is still a major unresolved problem in high-energy and plasma as trophysics. The diffusive/Fermi shock acceleration under turbulent fields has been discussed as one of important processes in the production of the high-energy particles, but alternative mechanisms that can accelerate particles in a short time scale have been recently discussed as efficient non-thermal particle acceleration mechanisms. First we review the standard diffusive/Fermi acceleration, and then discuss new ideas involving the direct/fast acceleration mechanisms of the magnetic reconnection and the electron shock surfing process.
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The origin of high energy particles seen radiating in astrophysical synchrotron sources is still a major unresolved problem in high-energy and plasma as trophysics. The diffusive/Fermi shock acceleration under turbulent fields has been discussed as one of important processes in the production of the high-energy particles, but alternative mechanisms that can accelerate particles in a short time scale have been recently discussed as efficient non-thermal particle acceleration mechanisms. First we review the standard diffusive/Fermi acceleration, and then discuss new ideas involving the direct/fast acceleration mechanisms of the magnetic reconnection and the electron shock surfing process.
Key concepts: Physics, Fermi acceleration, Particle acceleration, Cosmic ray, Acceleration, Plasma, Shock waves in astrophysics, Relativistic particle