Self-modulation of nonlinear Alfven waves in a strongly magnetized relativistic electron-positron plasma

被引:17
|
作者
Lopez, Rodrigo A. [1 ]
Asenjo, Felipe A. [2 ]
Munoz, Victor [1 ]
Chian, Abraham C. -L. [3 ,4 ,5 ]
Valdivia, J. A. [1 ,6 ,7 ]
机构
[1] Univ Chile, Fac Ciencias, Dept Fis, Santiago, Chile
[2] Univ Texas Austin, Inst Fus Studies, Austin, TX 78712 USA
[3] Observ Paris, CNRS, F-92195 Meudon, France
[4] Natl Inst Space Res INPE, Sao Jose Dos Campos, SP, Brazil
[5] WISER, Sao Jose Dos Campos, SP, Brazil
[6] CEDENNA, Ctr Desarrollo Nanociencia & Nanotecnol, Santiago, Chile
[7] CEIBA Complejidad, Bogota, Colombia
来源
PHYSICAL REVIEW E | 2013年 / 88卷 / 02期
关键词
HOT ACCRETION DISKS; PAIR PLASMA; PARTICLE-ACCELERATION; CURRENT SHEETS; RECONNECTION; MAGNETOSPHERES; OUTFLOW;
D O I
10.1103/PhysRevE.88.023105
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
We study the self-modulation of a circularly polarized Alfven wave in a strongly magnetized relativistic electron-positron plasma with finite temperature. This nonlinear wave corresponds to an exact solution of the equations, with a dispersion relation that has two branches. For a large magnetic field, the Alfven branch has two different zones, which we call the normal dispersion zone (where d omega/dk > 0) and the anomalous dispersion zone (where d omega/dk < 0). A nonlinear Schrodinger equation is derived in the normal dispersion zone of the Alfven wave, where the wave envelope can evolve as a periodic wave train or as a solitary wave, depending on the initial condition. The maximum growth rate of the modulational instability decreases as the temperature is increased. We also study the Alfven wave propagation in the anomalous dispersion zone, where a nonlinear wave equation is obtained. However, in this zone the wave envelope can evolve only as a periodic wave train.
引用
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页数:8
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