Equilibrium of Gravitating System of Spherical Gas-Dust Cloud

M. Abobaker
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Abstract

In this paper, we take several different analytical and numerical approaches to studying the equilibrium of a gravitating system of a gas-dust cloud. We consider one-dimensional self-gravitating spherically symmetric fluid flow of a gas-dust cloud. We discuss the equilibrium of the system of gas-dust cloud by using simplified analytic stellar, polytropic models. A condition for the equilibrium of the cloud in the form of a differential equation is used. Using mass density in the cloud as a given function, we obtained the corresponding pressure analytically within the cloud and determined the central pressure. In dealing with a polytropic model, we found the analytical and numerical solution of the Lane-Emden equation for the various values of the polytropic index after that, central density and central pressure were obtained. Finally, the density and pressure of the cloud for the various values of the polytropic index are calculated. The result found by the simplified analytical method and the polytropic method is compared.
球形气尘云引力系统的平衡
在本文中,我们采用几种不同的解析和数值方法来研究气尘云引力系统的平衡。我们考虑一维自重力球对称气体尘埃云的流体流动。我们用简化的解析恒星多向模型讨论了气尘埃云系统的平衡。用微分方程的形式给出了云的平衡条件。以云中质量密度为给定函数,解析得到云中相应的压力,并确定中心压力。在处理多向性模型时,得到了多向性指数各值的Lane-Emden方程的解析解和数值解,得到了中心密度和中心压力。最后,计算了不同多向性指数值下云的密度和压力。比较了简化分析方法和多向分析方法的结果。
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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