Propagation of symmetric and anti-symmetric surface waves in aself-gravitating magnetized dusty plasma layer with generalized (r, q) distribution

2018 ◽  
Vol 25 (5) ◽  
pp. 053704 ◽  
Author(s):  
Myoung-Jae Lee ◽  
Young-Dae Jung
Keyword(s):  
Surface Waves ◽  
Dusty Plasma ◽  
Plasma Layer ◽  
Magnetized Dusty Plasma ◽  
Symmetric Surface

Alfvén surface waves in a magnetized dusty plasma

1996 ◽  
Vol 3 (12) ◽  
pp. 4740-4747 ◽  
Author(s):  
N. F. Cramer ◽  
S. V. Vladimirov
Keyword(s):  
Surface Waves ◽  
Dusty Plasma ◽  
Magnetized Dusty Plasma

Low frequency surface waves in the magnetized dusty plasma

1998 ◽  
Vol 46 (4) ◽  
pp. 399-403 ◽  
Author(s):  
A.N. Kotsarenko ◽  
N.Ya. Kotsarenko ◽  
S.A. Silich
Keyword(s):  
Surface Waves ◽  
Dusty Plasma ◽  
Low Frequency ◽  
Magnetized Dusty Plasma

Gravitating–radiative magnetohydrodynamic surface waves

2020 ◽  
Vol 86 (4) ◽  
Author(s):  
R. Ruby ◽  
Ch. Rozina ◽  
N. L. Tsintsadze ◽  
Z. Iqbal
Keyword(s):  
Thermal Radiation ◽  
Surface Waves ◽  
Dusty Plasma ◽  
Temperature Inhomogeneity ◽  
Charged Surface ◽  
Linear Dispersion ◽  
Surface Mass ◽  
Magnetized Dusty Plasma ◽  
Vacuum Interface ◽  
Astrophysical Objects

Radiative-magnetohydrodynamic (RMHD) equations along with a full set of Maxwell's equations are followed to formulate the charged surface waves at the interface of an incompressible, radiative, magnetized dusty plasma and vacuum, while assuming that the characteristic wave frequency is much smaller than the ion gyrofrequency, having an equilibrium background state. It is found that the separation of charges on the surface is followed by thermal motion, which further leads to a negative pressure gradient normal to the surface, hence the plasma–vacuum interface is under tension due to two different types of oppositely directed pressures. The dusty plasma RMHD set of equations admits a linear dispersion relation of surface Jeans instability of an incompressible dusty plasma, which exhibits a strong coupling between the electron surface charge and dust surface mass densities and we conclude that the surface densities of both electrons and dust as well as the dust inertia play major roles in the gravitational collapse of the surface of astrophysical objects such as stars, galaxies etc. Further, the growth rate of radiative surface waves is found to be function of both the temperature inhomogeneity, appearing due to thermal radiation heat flux, as well as the thermal radiation pressure. The present findings of charged surface waves may seek application at the astroscales.

scholarly journals Low-frequency surface waves in a structured magnetized dusty plasma

1999 ◽  
Vol 104 (A1) ◽  
pp. 593-596 ◽  
Author(s):  
K. N. Ostrikov ◽  
S. V. Vladimirov ◽  
M. Y. Yu
Keyword(s):  
Surface Waves ◽  
Dusty Plasma ◽  
Low Frequency ◽  
Magnetized Dusty Plasma

Dust acoustic surface waves on a dusty plasma slab

2000 ◽  
Vol 7 (6) ◽  
pp. 2731-2732 ◽  
Author(s):  
L. Stenflo ◽  
P. K. Shukla ◽  
M. Y. Yu
Keyword(s):  
Surface Waves ◽  
Dusty Plasma ◽  
Dust Acoustic ◽  
Plasma Slab ◽  
Acoustic Surface Waves

Surface Waves at a Dusty Plasma-Metal Interface

2004 ◽  
Vol 70 (1) ◽  
pp. 33-37 ◽  
Author(s):  
Yu A Akimov ◽  
N A Azarenko ◽  
V P Olefir
Keyword(s):  
Surface Waves ◽  
Dusty Plasma ◽  
Metal Interface
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