Abstract

Linear and nonlinear coupled kinetic Alfven acoustic (CKAA) waves in low-β electron–positron–ion (e-p-i) plasmas are investigated in this paper, and the main focus is on highlighting the role of non-thermal electrons and positrons that follow the generalized (r, q) distribution. In this regard, a linear dispersion relation is derived, and the effect of positron concentration and (r, q) distributed electrons and positrons is explored. Nonlinear analysis is performed by using the Sagdeev potential approach and two-potential theory. The results are compared with those of the previous studies of CKAA waves in e-p-i plasmas where electrons and positrons follow Maxwellian and kappa distributions. An important feature of our study is the observation of the existence of density dip solitons for spiky distribution. It is shown that the inclusion of positrons alters the existence regimes of the solitary structures, and, interestingly, the behavior of soliton propagation is different in the two existence regimes for increasing or decreasing concentration of positrons. Most importantly, it is shown that the spatial scales over which solitons form in e-p-i plasmas are shorter than the ones that form in e-i plasmas for compressive solitary structures. Interestingly, the situation is reversed for rarefactive solitary structures. The present study is beneficial in comprehending the linear and nonlinear propagation of CKAA waves in plasmas where positrons are present, and there is a simultaneous presence of nonthermal features in the observed distribution functions.

Highlights

  • Electron–positron–ion (e-p-i) plasmas are known to play a marked role in the realm of plasma physics because of their existence in early universe astrophysical plasmas,[1] magnetospheres of pulsars,[2] solar atmosphere,[3] and active galactic nuclei.[4]

  • The linear dispersion relation of coupled kinetic Alfven acoustic (CKAA) waves, Eq (17), is rearranged and plotted in Fig. 1 such that frequency is normalized by ion cyclotron frequency and the wave number is normalized by the ion Larmor radius

  • This paper presents detailed analysis of coupled kinetic Alfven acoustic (CKAA) waves in three-component e-p-i plasmas

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Summary

INTRODUCTION

Electron–positron–ion (e-p-i) plasmas are known to play a marked role in the realm of plasma physics because of their existence in early universe astrophysical plasmas,[1] magnetospheres of pulsars,[2] solar atmosphere,[3] and active galactic nuclei.[4]. Kinetic Alfven waves (KAWs) have long been linked with energy transfer mechanisms in space and laboratory plasmas These waves may cause turbulent heating in the solar wind and magnetosheath,[22] drive energy into Earth’s auroral regions, causing outflow of charged particles, and transfer undesirable energy from core regions to the reactor edges of fusion plasmas. We have focused on exploring the influence of positron concentration and the nonthermal parameters r and q on the propagation characteristics of solitary structures

GOVERNING SET OF EQUATIONS
LINEAR ANALYSIS
NONLINEAR ANALYSIS
RESULTS AND DISCUSSION
CONCLUSION
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