On the stability of two-dimensional modulated electrostatic wavepackets in non-Maxwellian dusty plasma-application in Saturn's magnetosphere
Kuldeep Singh, Michael McKerr, and Ioannis Kourakis

TL;DR
This study investigates the stability of two-dimensional electrostatic wavepackets in non-Maxwellian dusty plasmas, revealing how dust charge influences modulational instability, with implications for Saturn's magnetosphere observations.
Contribution
It introduces a 3D Davey-Stewartson model for dusty plasmas with suprathermal electrons, analyzing modulational stability differences based on dust charge, which was not previously explored.
Findings
Negative dust suppresses modulational instability.
Positive dust enhances instability growth rate.
Instability criteria differ from Maxwellian plasma predictions.
Abstract
Motivated by observations of localized electrostatic wavepackets by the Voyager 1 and 2 and Cassini missions in Saturn's magnetosphere, we have investigated the evolution of modulated electrostatic wavepackets in a dusty plasma environment. The well-known dust-ion acoustic (DIA) mode was selected to explore the dynamics of multi-dimensional structures, by means of a Davey-Stewartson (DS) model, by taking into account the presence of a highly energetic (suprathermal, kappa-distributed) electron population in combination with heavy (immobile) dust in the background. The modulational (in)stability profile of DIA wavepackets for both negative as well as positive dust charge is investigated. A set of explicit criteria for modulational instability (MI) to occur is obtained. Wavepacket modulation properties in 3D dusty plasmas are shown to differ from e.g. Maxwellian plasmas in 1D. Stronger…
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