Volume 65, Issue 3 e202400008
ORIGINAL ARTICLE

Amplitude modulation and nonlinear dynamics of small amplitude ion-acoustic waves in five component cometary plasmas

Debaditya Kolay

Debaditya Kolay

Department of Basic and Applied Science, National Institute of Technology Arunachal Pradesh, Jote, India

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Debjit Dutta

Corresponding Author

Debjit Dutta

Department of Basic and Applied Science, National Institute of Technology Arunachal Pradesh, Jote, India

Correspondence

Debjit Dutta, Department of Basic and Applied Science, National Institute of Technology Arunachal Pradesh, Jote 791113, India.

Email: [email protected]

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Biswajit Sahu

Biswajit Sahu

Department of Mathematics, West Bengal State University, Kolkata, India

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First published: 22 May 2024
Citations: 2

Abstract

The formation and propagation dynamics of the finite-amplitude ion-acoustic wave (IAW) structures (e.g., soliton, breather, rogue wave, etc.) is theoretically investigated in a plasma comprising of kappa distributed solar and cometary electrons of different temperatures, a hot H 3 O + $$ {\mathrm{H}}_3{\mathrm{O}}^{+} $$ drift ion component, and a pair of oppositely charged oxygen ion components. The modified-KdV (mKdV) equation is derived in order to study the propagation dynamics of the ion-acoustic solitary wave (IASW). It is then converted into the nonlinear Schrödinger equation (NLS) through appropriate algebraic manipulation in order to observe the amplitude modulation of the IAWs. Also, the appearance of envelope soliton and the possibility of breather structure formation have been studied from the NLS equation. The dependence of plasma parameters on the formation and propagation of IAW structures has been briefly discussed. The modified-KdV equation is reduced in a dynamical system through the application of coordinate transformation. The existence of finite-amplitude nonlinear and supernonlinear IAWs is demonstrated by phase plane analysis. Due to the fact that the results are primarily associated with cometary plasma, they possibly provide greater insight of the nonlinear characteristics of cometary plasma.

CONFLICT OF INTEREST STATEMENT

The authors declare that they have no competing interests.

DATA AVAILABILITY STATEMENT

Data sharing not applicable to this article as no datasets were generated or analysed during the current study.

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