# Dust-acoustic envelope solitons and rogue waves in an electron depleted   plasma

**Authors:** J. Akter, N. A. Chowdhury, and A. A. Mamun

arXiv: 1907.11522 · 2019-07-29

## TL;DR

This paper theoretically studies dust acoustic wave modulation, envelope solitons, and rogue waves in an electron-depleted dusty plasma, revealing how plasma parameters influence wave stability and structure.

## Contribution

It derives a nonlinear Schrödinger equation for dust acoustic waves in electron-depleted plasma and identifies conditions for solitons and rogue waves, considering various plasma parameters.

## Key findings

- Identification of conditions for bright and dark solitons.
- Discovery of criteria for rogue wave formation.
- Influence of plasma parameters on wave stability.

## Abstract

Theoretical investigation of the nonlinear propagation and modulational instability (MI) of the dust acoustic (DA) waves (DAWs) in an unmagnetized electron depleted dusty plasma (containing opposite polarity warm dust grains and non-extensive positive ions) has been made by deriving a nonlinear Schr\"{o}dinger equation with the help of perturbation method. Two types of mode, namely, fast and slow DA modes, have been found. The criteria for the formation of bright and dark envelope solitons as well as the first-order and second-order rogue waves have been observed. The effects of various dusty plasma parameters (viz., dust mass, dust charge, dust and ion number densities, etc.) on the MI of DAWs have been identified. It is found that these dusty plasma parameters significantly modify the basic features of the DAWs. The applications of the results obtained from this theoretical investigation in different regions of space, viz., magnetosphere of Jupiter, upper mesosphere, Saturn's F-ring, and cometary tail, etc.

## Full text

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## Figures

14 figures with captions in the complete paper: https://tomesphere.com/paper/1907.11522/full.md

## References

54 references — full list in the complete paper: https://tomesphere.com/paper/1907.11522/full.md

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Source: https://tomesphere.com/paper/1907.11522