2014
DOI: 10.1063/1.4863848
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Shock waves and double layers in electron degenerate dense plasma with viscous ion fluids

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Cited by 20 publications
(11 citation statements)
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“…It is well known that in a nonlinear dispersive media shock waves are formed due to an interplay between the nonlinearity (causing wave steepening) and dissipation (e.g., caused by viscosity, collisions, wave particle interaction, etc.) [19][20][21][22]. However, when a medium exhibits both dispersive and dissipative properties, the propagation characteristics of small-amplitude perturbations can be adequately described by KdVB (in one-dimension) or KPB (in two or three dimensios) equations.…”
Section: Introductionmentioning
confidence: 99%
See 1 more Smart Citation
“…It is well known that in a nonlinear dispersive media shock waves are formed due to an interplay between the nonlinearity (causing wave steepening) and dissipation (e.g., caused by viscosity, collisions, wave particle interaction, etc.) [19][20][21][22]. However, when a medium exhibits both dispersive and dissipative properties, the propagation characteristics of small-amplitude perturbations can be adequately described by KdVB (in one-dimension) or KPB (in two or three dimensios) equations.…”
Section: Introductionmentioning
confidence: 99%
“…[19][20][21][22]. However, when a medium exhibits both dispersive and dissipative properties, the propagation characteristics of small-amplitude perturbations can be adequately described by KdVB (in one-dimension) or KPB (in two or three dimensios) equations.…”
Section: Introductionmentioning
confidence: 99%
“…To do so, we employ a reductive perturbation technique to examine the electrostatic perturbation propagating in a dense electronpositron degenerate plasma system due to the effect of dissipation. Now, we first introduce the stretched coordinates [15] …”
Section: Derivation Of Modified Burgers Equationmentioning
confidence: 99%
“…For describing and analyzing the different astrophysical environments [14][15][16] (where particle velocities are close to the speed of light), relativistic degeneracy of plasmas has received a great attention and relativistic effects [17][18][19][20][21] play an important role in understanding the different electrostatic nonlinear phenomena. Plasmas in different astrophysical compact objects such as white dwarfs, neutron stars, and so on are examples where relativistic degeneracy is a dominant phenomenon.…”
Section: Introductionmentioning
confidence: 99%
“…So, a purely one-dimensional model can account for none of all observed features since the wave structure and many properties of the solitary waves are modified by these transverse perturbations. [46,47] Motivated by these observations, Zobaer et al [48] and Mamun and Zobaer [49] derived first a modified Burgers equations in the planar case with adiabatic pressure; however, very few investigations have been done on the derivations of a two-dimensional Burgers equations. [50] Furthermore to the best of our knowledge, no observation has been reported on three-dimensional (3D) Burgers equations except a few observations by this author.…”
Section: Introductionmentioning
confidence: 99%