Spherical nonthermal pulsational mode stability thermo-statistically moderated with extra-negative ions

Jonmoni Dutta , Ahmed Atteya , Pralay Kumar Karmakar
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Abstract

The presence of diverse negative ions is well-known to modify different collective waves and instabilities in diverse space and astrophysical environments. We herein investigate the stability dynamics of the spherical nonthermal (kappa-modified) pulsational mode of gravitational collapse (PMGC) excitable in astrophysical dust molecular clouds (DMCs). It primarily explores the impact of the realistic nonthermal negative ionic effects on the PMGC stability features. The high-energetic lighter constituents, such as the electrons, positive ions, and negative ions, are modelled with their respective nonthermal kappa (κ)-distribution laws. The inertial dust particulates are treated in the viscous fluid fabric. Application of spherical normal mode treatment results in a generalized linear quartic (degree-4) dispersion relation. A computational illustrative platform illuminates the underlying stabilizing and destabilizing factors. It is seen that the cloud size, dust mass, dust charge, nonthermality parameters, equilibrium charged dust number density, and neutral dust viscosity play stabilizing roles. It counters the destabilizing scenarios caused by the equilibrium electron number density, positive ion number density, negative ion number density, neutral dust density, and charged dust viscosity. The fundamental physical mechanisms responsible herein are substantiated and compared in light of the previous predictions. The nontrivial avenues of our study in realizing the Jeans-driven galactic structural unit formation processes, moderated actively with the presence of negative ions in diverse real astronomical circumstances are summarily indicated.

Abstract Image

球面非热脉动模式稳定性与额外的负离子热统计缓和
众所周知,在不同的空间和天体物理环境中,不同负离子的存在会改变不同的集体波和不稳定性。本文研究了天体物理尘埃分子云(DMCs)中可激发的球形非热(kappa修正)引力坍缩(PMGC)脉动模式的稳定性动力学。主要探讨了实际非热负离子效应对PMGC稳定性特性的影响。高能量较轻的组分,如电子、正离子和负离子,用它们各自的非热kappa (κ)分布规律进行建模。惯性粉尘颗粒在粘性流体结构中进行处理。应用球面正模处理得到广义线性四次(4次)色散关系。计算说明平台阐明了潜在的稳定和不稳定因素。可见,云量、粉尘质量、粉尘电荷、非热性参数、平衡带电尘数密度和中性尘粘度均起稳定作用。它抵消了由平衡电子数密度、正离子数密度、负离子数密度、中性粉尘密度和带电粉尘粘度引起的不稳定情况。根据先前的预测,本文证实并比较了其中的基本物理机制。摘要指出了我们在实现jean驱动的星系结构单元形成过程中的非平凡研究途径,这些过程在各种实际天文环境中受到负离子的积极调节。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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