Abstract:The existence of standing high frequency electromagnetic (EM) solitons in a fully degenerate overdense electron plasma is studied applying relativistic hydrodynamics and Maxwell equations. The stable soliton solutions are found in both relativistic and nonrelativistic degenerate plasmas.A significant amount of recent publications describe electromagnetic (EM) waves in relativistic plasmas and majority of them discuss possible roles of these waves in different astrophysical phenomena. Highly relativistic plasma… Show more
The nonlinear interaction of intense linearly polarized electromagnetic waves (EMWs) with longitudinal electron density perturbations is revisited in relativistic degenerate plasmas. The nonlinear dynamics of the EMWs and the longitudinal field, driven by the EMW ponderomotive force, is governed by a coupled set of nonlinear partial differential equations. A numerical simulation of these coupled equations reveals that the generation of wakefields is possible in weakly relativistic degenerate plasmas with R0 ≡ pF /mc ≪ 1 and vg/c ∼ 1, where pF is the Fermi momentum, m is the mass of electrons, c is the speed of light in vacuum, and vg is the EMW group velocity. However, when the ratio vg/c is reduced to ∼ 0.1, the wakefield generation is suppressed, instead the longitudinal fields get localized to form soliton-like structures. On the other hand, in the regimes of moderate (R0 1) or strong relativistic degeneracy (R0 > 1) with vg/c ∼ 0.1, only the EM solitons can be formed.
The nonlinear interaction of intense linearly polarized electromagnetic waves (EMWs) with longitudinal electron density perturbations is revisited in relativistic degenerate plasmas. The nonlinear dynamics of the EMWs and the longitudinal field, driven by the EMW ponderomotive force, is governed by a coupled set of nonlinear partial differential equations. A numerical simulation of these coupled equations reveals that the generation of wakefields is possible in weakly relativistic degenerate plasmas with R0 ≡ pF /mc ≪ 1 and vg/c ∼ 1, where pF is the Fermi momentum, m is the mass of electrons, c is the speed of light in vacuum, and vg is the EMW group velocity. However, when the ratio vg/c is reduced to ∼ 0.1, the wakefield generation is suppressed, instead the longitudinal fields get localized to form soliton-like structures. On the other hand, in the regimes of moderate (R0 1) or strong relativistic degeneracy (R0 > 1) with vg/c ∼ 0.1, only the EM solitons can be formed.
“…In a series of papers [5]- [8], where authors examined the nonlinear character of interactions of plasma waves and high frequency EM waves it was found that ✩ Fully documented templates are available in the elsarticle package on CTAN.…”
Section: Introductionmentioning
confidence: 99%
“…In the present paper, we apply the fluid-Maxwell model developed in [5], [7] to study the possibility of FI of intense narrow electromagnetic pulse L ⊥ << L (where L and L ⊥ are the characteristic longitudinal and transverse spatial dimensions of the field, respectively) in the transparent degenerate electron plasma to show the possibility of FI in relativistic degenerate plasma embedded in the field of arbitrary strong EM radiation.…”
The filamentation instability of the electromagnetic (EM) beam in an underdense plasma with high level of degeneracy is examined by means of the momentum equation, continuity equation and Maxwell's equations. It has been demonstrated that the instability develops for weakly as well as strongly relativistic degenerate plasma and arbitrary strong amplitude of EM beams.
“…For discussion on the formation and features of EM soliton, the Maxwell and fluid equations should be solved. A multiple scales technique is used to solve the fluid-Maxwell equations in cold plasma [10][11][12][13][14]. Kuehl and Zhang [15] have expressed the creation of bright and dark EM soliton in weakly relativistic approximation.…”
The nonlinear Schrödinger equation (NLS) that describes the propagation of high intensity laser pulse through plasma is obtained by employing the multiple scales technique. One of the arresting solution for NLS equation is soliton like envelope for vector potential that is called electromagnetic soliton. The type and amplitude of electromagnetic soliton (EM) depends on the distribution function of plasma's particles. In this paper, distribution function of electrons obey the Cairns-Tsallis model and ions are assumed as stationary background. There are two flexible parameters, affect on the formation of EM soliton. By variation of nonextensive and nonthermal parameters, bright soliton could convert to dark one or versus. Due to positive kinetic energy, there are the limited region for nonextensive and nonthermal parameters as q [ 0.6 and 0 \ a \ 0.25. The variation of EM soliton's amplitude is discussed analytically.
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