Instability of dust-ion acoustic solitary waves in a collisionless magnetized five components plasma

被引:2
|
作者
Halder, P. [1 ]
Bandyopadhyay, A. [1 ]
Sardar, S. [2 ]
机构
[1] Jadavpur Univ, Dept Math, Kolkata 700032, India
[2] Guru Ghasidas Vishwavidyalaya, Dept Math, Bilaspur 495009, India
关键词
Instability; DIA solitary waves; Five components e-p-i-d plasma; Small-k perturbation expansion method; ZAKHAROV-KUZNETSOV EQUATION; MULTIDIMENSIONAL INSTABILITY; STABILITY ANALYSIS; KINETIC ALFVEN; NONTHERMAL PLASMA; PAINLEVE ANALYSIS; KP EQUATION; GROWTH-RATE; SOLITONS; KDV;
D O I
10.1007/s12648-023-02839-0
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
In the present paper, we have discussed the stability of dust-ion acoustic solitary waves obtained from the Korteweg-de Vries-Zakharov-Kuznetsov (KdV-ZK) equation and different modified KdV-ZK equations derived in the recent paper of Halder et al. (Z Naturforsch A 77:659, 2022) in a collisionless magnetized five components electron-positron-ion-dust plasma system consisting of warm adiabatic ions, Cairns distributed nonthermal positrons, Maxwellian distributed cold isothermal electrons, Cairns distributed nonthermal electrons and negatively charged static dust grains. We have used the small-k perturbation expansion method of Rowlands and Infeld (J Plasma Phys 3:567, 1969, J Plasma Phys 8:105, 1972, J Plasma Phys 10:293, 1973, J Plasma Phys 33:171, 1985) to analyze the stability of the steady state solitary wave solution of the KdV-ZK equation and different modified KdV-ZK equations. In this method, we want to find a nonlinear dispersion relation of the nonlinear evolution equation connecting the lowest order of & omega; and k, where & omega; is the wave frequency and k is the wave number. This nonlinear dispersion relation helps to analyze the stability of solitary structures of the KdV-ZK equation and different modified KdV-ZK equations. We have found the instability condition and the growth rate of instability up to the lowest order of wave number (k). We have graphically analyzed the growth rate of instability of different evolution equations with respect to different parameters of the present plasma system.
引用
收藏
页码:771 / 783
页数:13
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