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Research Article

Instability of opposite polarity charged dusty plasma with vortex-like distributed electrons

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Pages 351-361 | Received 29 Jun 2020, Accepted 24 Mar 2022, Published online: 08 Apr 2022
 

Abstract

Electrons in space plasma may follow vortex-like distribution, that is why we have derived the three-dimentional (3D) nonlinear modified Zakharov–Kuznetsov (mZK), describing the propagation of dust acoustic solitary to the plasma system composed of four components, magnetized charged dust plasma with electrons modelled by vortex-like distribution. By using the reductive perturbation method, it has been found that both solitary wave amplitude and width are affected by the plasma parameters: graim charge ratio ρ, population parameter β, and temperature ratio σ. The small-k perturbation technique has also been applied to study the instability criterion and growth rate of this instability. Cyclotron frequency Ω, temperature ratio σd, direction cosine (ιη and ιζ), and grain charge ratio ρ are found to modify the instability growth rate Γ.

Disclosure statement

No potential conflict of interest was reported by the author(s).