Abstract:The theoretical investigation of shocks and solitary structures in a dense quantum plasma containing electrons at finite temperature, nondegenerate cold electrons, and stationary ions has been carried out. A linear dispersion relation is derived for the corresponding electron acoustic waves. The solitary structures of small nonlinearity have been studied by using the standard reductive perturbation method. We have considered collisions to be absent, and the shocks arise out of viscous force. Furthermore, with … Show more
“…In this whole discussion, we have considered the ion velocity at about ten times greater than the velocity of dust particles. As we said in the previous result that we have discussed most of the results in the supersonic region so the effect of the dust streaming velocity is very less but it is the opposite of the result previously found for electro-static [16] or electron-acoustic [48,49] cases. In these papers, when the streaming velocities of the constituent particles increase the nonlinearity decrease, and the dispersive effect increases significantly.…”
Section: Resultscontrasting
confidence: 62%
“…There are two kinds of shock that can form in the case of fluids the first and mostly found in a viscous plasma is the strong shock when two fluids are propagating or colliding with each other with a velocity greater than the local acoustic waves, i.e. (M > 1) and the second kind of shock when two fluids collide a subsonic speed (M < 1) which is known as weak shock, this type of shock is very well known in case of fluids [64,65] and for laser-plasma interaction [16] but till now no report has been made in the case of dusty plasma. In figure 5 Now as we have discussed in section 4.2 when there is no viscous term the KdVB transforms into the KdV equation and here we will discuss the analytical solution of the KdV equation, i.e the solitary waves.…”
Section: Resultsmentioning
confidence: 99%
“…Applying this pressure term without considering the Bohm diffraction term we get the equation (3). Following the same procedure as used by Akbari-Moghanjoughi and Eliasson [42] and Goswami et al [16] we get the σ as…”
Section: The Finite Temperature Correction In the Ionmentioning
confidence: 99%
“…Furthermore, the ion-acoustic (IA) [14], electron acoustic (EA) [15] and electron-static (ES) [16] modes can also be present in a dusty plasma environment.…”
A viscous dusty plasma containing Kappa-(κ−) distributed electrons,positive warm viscous ions and constant negatively charged dust grains with viscosity have been considered to study the modes of dust-ion-acoustic waves (DIAWs) theoretically and numerically. The derivations and basic features of shock and solitary waves with different plasma parameters like Mach number, finite temperature coefficient, unperturbed dust streaming velocity, kinematic viscosity of dust etc. of this DIAWs mode have been performed. Considering the dynamical equation from Korteweg–de Vries(KdV) equation, a phase portrait has been drawn and the position of saddle point or col. and center have also been discussed. This type of dusty plasma can be found in celestial bodies. The results of this research work can be applied to study the properties of DIAWs in various astrophysical situation where κ-distributive electrons are present and careful modification of the same model can help us to understand the nature of the DIAWs of laboratory plasma as well.
“…In this whole discussion, we have considered the ion velocity at about ten times greater than the velocity of dust particles. As we said in the previous result that we have discussed most of the results in the supersonic region so the effect of the dust streaming velocity is very less but it is the opposite of the result previously found for electro-static [16] or electron-acoustic [48,49] cases. In these papers, when the streaming velocities of the constituent particles increase the nonlinearity decrease, and the dispersive effect increases significantly.…”
Section: Resultscontrasting
confidence: 62%
“…There are two kinds of shock that can form in the case of fluids the first and mostly found in a viscous plasma is the strong shock when two fluids are propagating or colliding with each other with a velocity greater than the local acoustic waves, i.e. (M > 1) and the second kind of shock when two fluids collide a subsonic speed (M < 1) which is known as weak shock, this type of shock is very well known in case of fluids [64,65] and for laser-plasma interaction [16] but till now no report has been made in the case of dusty plasma. In figure 5 Now as we have discussed in section 4.2 when there is no viscous term the KdVB transforms into the KdV equation and here we will discuss the analytical solution of the KdV equation, i.e the solitary waves.…”
Section: Resultsmentioning
confidence: 99%
“…Applying this pressure term without considering the Bohm diffraction term we get the equation (3). Following the same procedure as used by Akbari-Moghanjoughi and Eliasson [42] and Goswami et al [16] we get the σ as…”
Section: The Finite Temperature Correction In the Ionmentioning
confidence: 99%
“…Furthermore, the ion-acoustic (IA) [14], electron acoustic (EA) [15] and electron-static (ES) [16] modes can also be present in a dusty plasma environment.…”
A viscous dusty plasma containing Kappa-(κ−) distributed electrons,positive warm viscous ions and constant negatively charged dust grains with viscosity have been considered to study the modes of dust-ion-acoustic waves (DIAWs) theoretically and numerically. The derivations and basic features of shock and solitary waves with different plasma parameters like Mach number, finite temperature coefficient, unperturbed dust streaming velocity, kinematic viscosity of dust etc. of this DIAWs mode have been performed. Considering the dynamical equation from Korteweg–de Vries(KdV) equation, a phase portrait has been drawn and the position of saddle point or col. and center have also been discussed. This type of dusty plasma can be found in celestial bodies. The results of this research work can be applied to study the properties of DIAWs in various astrophysical situation where κ-distributive electrons are present and careful modification of the same model can help us to understand the nature of the DIAWs of laboratory plasma as well.
“…Depending on the inter-particle interaction, shocks are again classified into non-collisional and collisional types. In the absence of collisional effects, shocks experience instabilities due to collective phenomena in plasma which provide the excess energy to be dissipated at the shock front and in the presence of collisions the kinetic energy is supplied by the binary collisions and the shock fronts are narrower with a width of a few mean free path of binary collisions [6,7].…”
The characteristics of nonlinear electron-acoustic waves such as shocks and solitons, are investigated in a three component, dense laser produced plasma consisting of ions and two distinct groups of electrons, using the quantum hydrodynamic model and the standard reductive perturbation method. The modified Korteweg-deVries (mKdV) and Korteweg-deVries-Burgers (KdVB)equations have been derivedfor the electron-acoustic waves in the plasma. The dependence of both shocks and solitons on various parameters has been extensively studied. It is observed that whenever the density crosses the limit from the classical to the quantum range, the effective potential remains invariant for the solitary profiles; but shows a slight variation for the shock profiles. The collisional effect plays a significant role in the dissipation of solitary waves and the dissipation is larger for higher values of collision frequencies. The results obtained could prove helpful for understanding the parametric dependence of nonlinear waves in highly intense laser plasma interactions.
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