A new particle acceleration process in a developing Alfvén turbulence in the course of successive parametric instabilities of a relativistic pair plasma is investigated by utilizing one-dimensional electromagnetic full particle code. Coherent wave-particle interactions result in efficient particle acceleration leading to a power-law-like energy distribution function. In the simulation, high-energy particles having large relativistic masses are preferentially accelerated as the turbulence spectrum evolves in time. The main acceleration mechanism is simultaneous relativistic resonance between a particle and two different waves. An analytical expression of maximum attainable energy in such wave-particle interactions is derived.
CITATION STYLE
Matsukiyo, S., & Hada, T. (2009). Relativistic particle acceleration in developing Alfvén turbulence. Astrophysical Journal, 692(2), 1004–1012. https://doi.org/10.1088/0004-637X/692/2/1004
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