Transverse instability of ion acoustic solitons in a magnetized plasma including q-nonextensive electrons and positrons

被引:9
|
作者
Akhtar, N. [1 ,2 ]
El-Taibany, W. F. [3 ,4 ]
Mahmood, S. [1 ,2 ,5 ]
Behery, E. E. [3 ]
Khan, S. A. [5 ]
Ali, S. [5 ]
Hussain, S. [1 ,2 ]
机构
[1] PINSTECH, Theoret Phys Div TPD, Islamabad 44000, Pakistan
[2] PIEAS, Dept Phys & Appl Math DPAM, Islamabad 44000, Pakistan
[3] Damietta Univ, Fac Sci, Dept Phys, New Damietta, Egypt
[4] King Khalid Univ, Coll Sci Girls Abha, Dept Phys, Abha, Saudi Arabia
[5] Quaid I Azam Univ, Natl Ctr Phys NCP, Islamabad 44000, Pakistan
关键词
DOUBLE-LAYERS; SOLITARY WAVES; DISTRIBUTIONS; PROPAGATION; EQUATION; MODES; JET;
D O I
10.1017/S0022377815001038
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
A nonlinear Zakharov-Kuznetsov (ZK) equation for ion acoustic solitary waves (IASWs) is derived using the reductive perturbation method (RPM) for magnetized plasmas in which the inertialess electrons and positrons are nonextensively q-distributed while ions are assumed to be warm and inertial. It is found that both compressive as well as rarefactive solitons coexist in the present model for different regions of non-extensive electron and positron parameters, q(e) and q(p). The magnetic field has no effect on the amplitude of the IASW, whereas the obliqueness angle of the wave propagation, the ion-to-electron temperature ratio a and positron-to-ion density concentration ratio p affect both the amplitude and the width of the solitary wave structures. The transverse instability analysis illustrates that the one soliton solution has a constant growth rate, and it suffers from instability in the transverse direction. The relevance of the present study to astrophysical space plasmas is also discussed.
引用
收藏
页数:19
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