Landau damping of Gardner solitons in a dusty bi-ion plasma

TL;DR

This paper investigates how Landau damping influences the nonlinear propagation of dust-acoustic solitary waves in a dusty plasma with two ion species, deriving equations that describe their behavior and damping characteristics.

Contribution

It introduces a comprehensive analysis of Landau damping effects on Gardner solitons in a dusty bi-ion plasma, including derivation of governing equations and parameter-dependent damping features.

Findings

Gardner solitons exhibit lower amplitudes than KdV and mKdV solitons.

Landau damping causes decay in soliton amplitudes over time.

The damping rates depend on ion temperature ratios, densities, and mass ratios.

Abstract

The effects of linear Landau damping on the nonlinear propagation of dust-acoustic solitary waves (DASWs) are studied in a collisionless unmagnetized dusty plasma with two species of positive ions. The extremely massive, micron-seized, cold and negatively charged dust particles are described by fluid equations, whereas the two species of positive ions, namely the cold (heavy) and hot (light) ions are described by the kinetic Vlasov equations. Following Ott and Sudan [Phys. Fluids {\bf 12}, 2388 (1969)], and by considering lower and higher-order perturbations, the evolution of DASWs with Landau damping is shown to be governed by Korteweg-de Vries (KdV), modified KdV (mKdV) or Gardner (KdV-mKdV)-like equations. The properties of the phase velocity and the Landau damping rate of DASWs are studied for different values of the ratios of the temperatures $(\sigma)$ and the number densities $(\mu)$ of hot and cold ions as well the cold to hot ion mass ratio $m$. The distinctive features of the decay rates of the amplitudes of the KdV, mKdV and Gardner solitons with a small effect of Landau damping are also studied in different parameter regimes. It is found that the Gardner soliton points to lower wave amplitudes than the KdV and mKdV solitons. The results may be useful for understanding the localization of solitary pulses and associated wave damping (collisionless) in laboratory and space plasmas (e.g., the F-ring of Saturn) in which the number density of free electrons is much smaller than that of ions and the heavy, micron seized dust grains are highly charged.