Abstract:Modulation instability (MI) of envelope soliton is studied in an unmagnetized viscous plasma. Using Krylov-Bogoliubov Mitropolsky (KBM) method, the nonlinear Schrödinger equation (NLSE) is obtained, and the growth rate of modulationally unstable electron acoustic wave in such plasma is discussed. The solution of the electron-acoustic envelope-solitons is obtained from the Nonlinear Schrödinger equation. The hypothetical outcomes have been examined mathematically for various parameters of plasma, and the outcom… Show more
“…This law of force is known as 'Newton's law of viscosity'. In equations (2) and (3), the viscosity we use is the kinematic viscosity as we mentioned earlier and this is basically the ratio between absolute viscosity (μ) and fluid mass density (n), this is previously discussed by Goswami and Sarkar [39].…”
Section: The Kinematic Viscositymentioning
confidence: 99%
“…Then equation (33) transforms into the same form as equation (39) with a different F. This type of numerical solution for the KdVB equation is quite new. The solution of it following this procedure is given in Appendix A.2.…”
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.
“…This law of force is known as 'Newton's law of viscosity'. In equations (2) and (3), the viscosity we use is the kinematic viscosity as we mentioned earlier and this is basically the ratio between absolute viscosity (μ) and fluid mass density (n), this is previously discussed by Goswami and Sarkar [39].…”
Section: The Kinematic Viscositymentioning
confidence: 99%
“…Then equation (33) transforms into the same form as equation (39) with a different F. This type of numerical solution for the KdVB equation is quite new. The solution of it following this procedure is given in Appendix A.2.…”
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.
“…It is worth noting that there are multiple methods available to obtain NLSE, such as the reductive perturbation method, [51][52][53] Krylov-Bogoliubov-Mitropolsky (KBM) method, [54][55][56] canonical transformation method, [57] inverse scattering transform method, [58] and so on.…”
Present paper choose a dusty plasma as an example to numerically and analytically study the differences between two different methods of obtaining nonlinear Schrödinger equation (NLSE). The first method is to derive a Korteweg-de Vries (KdV) type equation and then derive the NLSE from the KdV type equation, while the second one is to directly derive the NLSE from the original equation. It is found that the envelope waves from the two methods have different dispersion relations, different group velocities. The results indicate that two envelope wave solution from two different methods are completely different. The results also show that the application scope of the envelope wave obtained from the second method is wider than that of the first method, though both methods are valuable in the range of their corresponding application scopes. It suggest that, for other system, both method to derive NLSE may be correct, but their nonlinear wave solutions are different and their application scopes are also different.
“…As it is known, the nonlinear Schrödinger equation (NLSE) is one of the equations applied to many physical problems in many fields. Such as quantum, atomic, water wave systems, plasma physics [1], nonlinear optics, etc. When this is the case, the most basic problem encountered is the formation of perturbations that cannot be integrated.…”
Section: Introductionmentioning
confidence: 99%
“…As it is well-known that the linear response of a medium to an electrical field described by P = ε 0 χ (1) E, which P, E, χ represent the polarization, electric field and linear response, respectively. If the strength of the applied electric field increases, the linear relationship given by P = ε 0 χ (1) E has to be generalized as, ( )…”
This article is dedicated to investigating a myriad of nonlinear forms of the resonant nonlinear Schrödinger equation, which is one of the essential examples of evolution equations, and providing some observations. The resonant nonlinear Schrödinger equation, in the presence of spatio-temporal and inter-modal dispersion, was addressed using the recently introduced Kudryashov’s method, and solution
functions were obtained for eleven different nonlinear forms (Kerr, power, parabolic, dual-power, polynomial, triple-power, quadratic-cubic, generalized quadratic-cubic, anti-cubic, generalized anti-cubic, and parabolic law with non-local nonlinearity). The study will contribute to the literature not only by examining such a diverse set of nonlinear forms together but also by investigating the impact of the degree of
nonlinearity and the coefficients of different nonlinearity terms on soliton behavior. Detailed examinations of all these points, the results obtained, observations, and necessary comments have been made in the relevant sections.
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