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Dust acoustic shock waves in dusty plasma of opposite polarity with non-extensive electron and ion distributions

Published online by Cambridge University Press:  25 March 2014

S. K. Zaghbeer ,
H. H. Salah ,
N. H. Sheta ,
E. K. El-Shewy  and
A. Elgarayhi
S. K. Zaghbeer
Affiliation:
Faculty of Science for Girls, Al-Azhar University, Nasr City, Cairo, Egypt
H. H. Salah
Affiliation:
Faculty of Science for Girls, Al-Azhar University, Nasr City, Cairo, Egypt
N. H. Sheta
Affiliation:
Faculty of Science for Girls, Al-Azhar University, Nasr City, Cairo, Egypt
E. K. El-Shewy
Affiliation:
Theoretical Physics Group, Faculty of Science, Mansoura University, Mansoura, Egypt
A. Elgarayhi*
Affiliation:
Theoretical Physics Group, Faculty of Science, Mansoura University, Mansoura, Egypt
*
†Email address for correspondence: [email protected]
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Abstract

A theoretical investigation has been made of obliquely propagating nonlinear electrostatic shock structures. The reductive perturbation method has been used to derive the Korteweg-de Vries-Burger (KdV-Burger) equation for dust acoustic shock waves in a homogeneous system of a magnetized collisionless plasma comprising a four-component dusty plasma with massive, micron-sized, positively, negatively dust grains and non-extensive electrons and ions. The effect of dust viscosity coefficients of charged dusty plasma of opposite polarity and the non-extensive parameters of electrons and ions have been studied. The behavior of the oscillatory and monotonic shock waves in dusty plasma has been investigated. It has been found that the presence of non-extensive parameters significantly modified the basic properties of shock structures in space environments.

Type
Papers
Information
Journal of Plasma Physics , Volume 80 , Issue 3 , June 2014 , pp. 517 - 528
Copyright
Copyright © Cambridge University Press 2014 

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