Quasilinear theory of general electromagnetic fluctuations in unmagnetized plasmas

被引:9
作者
Schlickeiser, R. [1 ,2 ]
Yoon, P. H. [3 ,4 ]
机构
[1] Ruhr Univ Bochum, Inst Theoret Phys, Lehrstuhl Weltraum & Astrophys 4, D-44780 Bochum, Germany
[2] Ruhr Univ Bochum, Res Dept Plasmas Complex Interact, D-44780 Bochum, Germany
[3] Univ Maryland, Inst Phys Sci & Technol, College Pk, MD 20742 USA
[4] Kyung Hee Univ, Sch Space Res, Yongin 446701, Gyeonggi Do, South Korea
基金
美国国家科学基金会; 新加坡国家研究基金会;
关键词
MAGNETIC-FIELD GENERATION; COLLISIONLESS SHOCKS;
D O I
10.1063/1.4893147
中图分类号
O35 [流体力学]; O53 [等离子体物理学];
学科分类号
070204 ; 080103 ; 080704 ;
摘要
The general quasilinear Fokker-Planck kinetic equation for the plasma particle distribution functions in unmagnetized plasmas is derived, making no restrictions on the frequency of the electromagnetic fluctuations. The derived kinetic particle equation complements our earlier study of the general fluctuation's kinetic equation. For collective plasma eigenmodes and gyrotropic particle distribution functions, the two coupled kinetic equations describe the self-consistent dynamical evolution of the plasma. The limit of weakly damped collective modes correctly reproduces the well-known textbook kinetic particle equation with longitudinal Langmuir and ion-acoustic fluctuations, demonstrating, in particular, the resonant nature of parallel momentum diffusion of particles. In the limit of aperiodic modes, the Fokker-Planck equation contains the nonresonant diffusion of particles in momentum and the parallel and perpendicular momentum drag coefficients. As an application these drag and diffusion coefficients are calculated for extragalactic cosmic ray particles propagating in the unmagnetized intergalactic medium. Whereas for all cosmic rays, the perpendicular momentum diffusion in intergalactic aperiodic fluctuations is negligibly small; cosmic ray protons with energies below 10(5) GeV are affected by the plasma drag. (C) 2014 AIP Publishing LLC.
引用
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页数:9
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