2008
DOI: 10.1063/1.2840642
|View full text |Cite
|
Sign up to set email alerts
|

Dust acoustic shock wave in electronegative dusty plasma: Roles of weak magnetic field

Abstract: The effects of nonsteady dust charge variations and weak magnetic field on small but finite amplitude nonlinear dust acoustic wave in electronegative dusty plasma are investigated. The dynamics of the nonlinear wave are governed by a Korteweg–de Vries Burger equation that possesses dispersive shock wave. The weak magnetic field is responsible for the dispersive term, whereas nonsteady dust charge variation is responsible for dissipative term, i.e., the Burger term. The coefficient of dissipative term depends o… Show more

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
2
1

Citation Types

0
20
0

Year Published

2011
2011
2023
2023

Publication Types

Select...
7

Relationship

2
5

Authors

Journals

citations
Cited by 25 publications
(20 citation statements)
references
References 27 publications
0
20
0
Order By: Relevance
“…However, in the presence of a very strong magnetic field, the orbits of the magnetized plasma particles are confined to one dimension along the field lines, and thus the perturbed field does not come into play, and the problem of charging currents becomes independent of the magnetic field. 25 The electron, negative ion, and positive ion charging currents ðI e ; I À ; I þ Þ for a spherical dust grain with radius r d are given by 5,15,17,22,26 …”
Section: Basic Equationsmentioning
confidence: 99%
See 2 more Smart Citations
“…However, in the presence of a very strong magnetic field, the orbits of the magnetized plasma particles are confined to one dimension along the field lines, and thus the perturbed field does not come into play, and the problem of charging currents becomes independent of the magnetic field. 25 The electron, negative ion, and positive ion charging currents ðI e ; I À ; I þ Þ for a spherical dust grain with radius r d are given by 5,15,17,22,26 …”
Section: Basic Equationsmentioning
confidence: 99%
“…Note that to justify the validity of our theoretical model, we consider a small deviation from the isothermal (Boltzmann) case ða ¼ 0Þ for the positive ions, i.e., 0 < a < 0: 15. We assume that the dust grain radius r d is much smaller than the electron gyroradius q e , 16,17,20,22,24 and that the dust flow velocity ( the thermal velocities V tj ðj ¼ e; þ; ÀÞ. As rightly pointed out by Taibany and Sabry, 17 this assumption (r d ( q e ) may be appropriate for a plasma laboratory that uses weak magnetic fields.…”
Section: Basic Equationsmentioning
confidence: 99%
See 1 more Smart Citation
“…To study small and finite-amplitude DMSW, we will use the reductive perturbation method [15] and introduce the stretched coordinates as…”
Section: Fast Time Scale Phenomenonmentioning
confidence: 99%
“…30,31 Recently, the dust acoustic shock wave due to nonadiabatic charge variations in a magnetized electronegative 1D dusty plasma is also investigated. 32 In this paper, we have investigated the effects of both adiabatic and nonadiabatic dust charge variations on nonlinear DAWs in a magnetized electronegative threedimensional (3D) dusty plasma using well known reductive perturbation technique (RPT). In case of adiabatic dust charge variations, we have obtained the ZakharovKuznetsov (ZK) equation which have usual solitary wave solutions.…”
Section: Introductionmentioning
confidence: 99%