Abstract

We present theoretical model analysis to study fully nonlinear behavior of gravito-electrostatic fluctuations in unmagnetized self-gravitating collisional dust cloud in presence of the ion-drag forces methodologically on the Jeans scales of space and time. The ion-drag effect as a result of streaming plasma ions arises here due to the ion orbital motion (scattering effect by dust) and the ion momentum transfer (capturing effect by dust) processes in opposite phase with the electrostatic force field. All the realistic astrophysical processes, such as electron impact-ionization of the neutral atoms, volume recombination, attachment of the electrons and ions to the dust grains and the collective plasma particle collisions are jointly considered. The Sagdeev pseudo-potential formulation is methodologically carried out in modified form to derive a new pair of gravito-electrostatically coupled energy integral equations. A numerical analysis is made to see the fluctuation features in judicious plasma parameter window. It is shown that the fluctuation dynamics evolves as self-gravitational rarefactive solitary structures and electrostatic compressive shock-like spectral patterns. The new features brought about by the considered ion-drag effects are discussed in the light of the existing theoretical, experimental and satellite-based predictions. The relevance of our results to understand the dynamics of self-gravitational collapse leading to galactic structure formation in interstellar space is briefly summarized.

Highlights

  • The study of nonlinear gravito-electrostatic waves, oscillations and fluctuations in self-gravitating dusty plasmas in the form of dust molecular clouds (DMCs) has been an importantly emerging area of great interest for years

  • Tions are governed by a new pair of gravito-electrostatically coupled energy integral equations (Eqs. (17)–(18)) by applying the Sagdeev pseudo-potential approach

  • We theoretically study the properties of fully nonlinear wave dynamics sourced by gravito-electrostatic coupling, in collisional, unmagnetized and self-gravitational dust cloud with the help of the Sagdeev pseudo-potential method

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Summary

Introduction

The study of nonlinear gravito-electrostatic waves, oscillations and fluctuations in self-gravitating dusty plasmas in the form of dust molecular clouds (DMCs) has been an importantly emerging area of great interest for years. It is seen that many authors have studied the evolutionary dynamics of various waves in different dusty plasma configurations with wide-range existence from laboratory to space in past They have found various structural waves which can either modify the original waves and instabilities or introduce new eigenmodes like solitons, shocks, double layers, vortices, etc. Rao et al have theoretically predicted the existence of the low-frequency dust-acoustic wave (DAW) in an unmagnetized dusty plasma by using the reductive perturbation technique (Rao et al 1990) They have showed that these waves propagate linearly as normal sound modes and nonlinearly as soliton-like eigenmodes, which arise due to the balance between nonlinear wave steepening and linear dispersion (Rao et al 1990). Shukla and Silin theoretically confirmed the existence of the low-frequency DAW (Shukla and Silin 1992)

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