Relativistic modulational instability of electron-acoustic waves in an electron-pair ion plasma

被引:20
|
作者
Misra, A. P. [1 ]
Shukla, P. K. [2 ,3 ,4 ,5 ,6 ,7 ,8 ,9 ,10 ]
机构
[1] Visva Bharati Univ, Dept Math, Santini Ketan 731235, W Bengal, India
[2] Ruhr Univ Bochum, Inst Theoret Phys 4, D-44780 Bochum, Germany
[3] Ruhr Univ Bochum, Ctr Plasma Sci & Astrophys, Fak Phys & Astron, D-44780 Bochum, Germany
[4] Ruhr Univ Bochum, Nonliner Phys Ctr, D-44780 Bochum, Germany
[5] Umea Univ, Dept Phys, SE-90187 Umea, Sweden
[6] Max Planck Inst Extraterr Phys, D-85741 Garching, Germany
[7] Inst Super Tecn, GoLP Inst Plasmas & Fusao Nucl, P-1049001 Lisbon, Portugal
[8] Rutherford Appleton Lab, CCLRC Ctr Fundamental Phys, Didcot OX11 0QX, Oxon, England
[9] Univ Strathclyde, SUPA Dept Phys, Glasgow G40NG, Lanark, Scotland
[10] COMSATS Inst Informat Technol, Dept Phys, Islamabad, Pakistan
关键词
modulational instability; plasma ion acoustic waves; plasma magnetohydrodynamics; plasma nonlinear processes; plasma simulation;
D O I
10.1063/1.3050062
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 modulational instability of finite amplitude electron-acoustic waves (EAWs) along the external magnetic field is studied in an electron-pair ion plasma. Accounting for the relativistic electron mass variation nonlinearity and the Boltzmann distribution of both positive and negative ions, new regimes for the relativistic modulational instability (MI) for the low frequency (below the electron gyrofrequency) short-wavelength (in comparison with the ion gyroradius) modes are obtained numerically. It is found that the presence of a significant fraction of negative ions suppresses the MI growth/decay rate for the modulated EAW packets. The results could be of important for understanding the origin of amplitude modulated EAW packets in space (e.g., Earth's magnetotail) as well as in laboratory plasmas.
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页数:5
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