Dust acoustic solitary waves in a five-component cometary plasma with charge variation

被引:0
作者
A. Varghese
A. C. Saritha
N. T. Willington
M. Michael
S. Sebastian
G. Sreekala
C. Venugopal
机构
[1] Mahatma Gandhi University,School of Pure and Applied Physics
[2] C M S College,Department of Physics
[3] Bharata Mata College,Department of Physics
[4] S B College,Department of Physics
[5] S D College,Department of Physics
来源
Journal of Astrophysics and Astronomy | 2020年 / 41卷
关键词
Charge varying dusty plasma; Lighter and heavier ions; Kappa described electrons; Rarefactive solitary waves;
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摘要
We studied dust acoustic solitary waves (DASW) in a five component cometary plasma by deriving the Kadomstev–Petiashvili (KP) equation. The five components consist of two components of electrons described by kappa distributions with different temperatures and spectral indices, a lighter (hydrogen) and a heavier (oxygen) ion component, both ion components are described by Maxwellian distributions. Dust particles, with varying charge, constitute the fifth component. The system supports rarefactive DASWs whose amplitudes are larger when the charges on the dust particles vary. The amplitudes also increase with increasing zd0nd0\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$ z_{d0} n_{d0} $$\end{document} (product of equilibrium charge number and density of dust) and increasing ion densities. It, however, decreases with increasing spectral indices of the electrons.
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