Space–time fractional KdV–Burgers equation for dust acoustic shock waves in dusty plasma with non-thermal ions

doi:10.1088/1674-1056/23/7/070505

Abstract The KdV-Burgers equation for dust acoustic waves in unmagnetized plasma having electrons, singly charged non-thermal ions, and hot and cold dust species is derived using the reductive perturbation method. The Boltzmann distribution is used for electrons in the presence of the cold (hot) dust viscosity coefficients. The semi-inverse method and Agrawal variational technique are applied to formulate the space-time fractional KdV-Burgers equation which is solved using the fractional sub-equation method. The effect of the fractional parameter on the behavior of the dust acoustic shock waves in the dusty plasma is investigated.

Keywords: dust-acoustic waves reductive perturbation method modified Riemann-Liouville fractional derivative space-time fractional KdV-Burgers equation

Received: 11 September 2013
Revised: 02 January 2014
Accepted manuscript online:

PACS:	05.45.Df	(Fractals)
	52.30.-q	(Plasma dynamics and flow)
	52.27.Lw	(Dusty or complex plasmas; plasma crystals)
	52.35.Fp	(Electrostatic waves and oscillations (e.g., ion-acoustic waves))

Corresponding Authors: Essam M. Abulwafa
E-mail: abulwafa@mans.edu.eg

About author: 05.45.Df; 52.30.-q; 52.27.Lw; 52.35.Fp

Cite this article:

Emad K. El-Shewy, Abeer A. Mahmoud, Ashraf M. Tawfik, Essam M. Abulwafa, Ahmed Elgarayhi Space–time fractional KdV–Burgers equation for dust acoustic shock waves in dusty plasma with non-thermal ions 2014 Chin. Phys. B 23 070505

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Space–time fractional KdV–Burgers equation for dust acoustic shock waves in dusty plasma with non-thermal ions

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