关于星系的气体动力学模型

Cai Shu-tang
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引用次数: 0

摘要

本文讨论了用于气体动力学模型的气体动力学方程的适用范围。指出(1)在处理引力坍缩时,当反应能量较大时,质量守恒定律和连续性方程不适用。(2)湍流的存在只影响基态运动。如果基态运动是给定的,如果我们忽略高阶小量,如果我们做一些简化的假设,那么小扰动的方程和没有湍流时的方程形式是一样的。C.C. Lin和他的同事所使用的方程正是小扰动的方程,因此即使存在湍流,Lin的理论仍然成立。如果我们希望得到下一个近似,那么我们通常必须考虑湍流。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
On gas dynamical models of galaxies

This paper discussed the range of applicability of the gas dynamical equations used in gas dynamical models. It is pointed out that (1), when dealing with gravitational collapse, the law of mass conservation and the equation of continuity are inapplicable if the reaction energies are large. (2) The presence of turbulence only affects the basic-state motion. If the basic-state motion is given and if we neglect higher-order small quantities and if we make certain simplifying assumptions, then the equations for small perturbations are of the same form as in the absence of turbulence. The equations used by C.C. Lin and his coworkers are precisely equations for small perturbations, hence Lin's theory still holds even if there is turbulence. If we wish to go to the next approximation, then we must, in general, take account of turbulence.

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