自引力理想气体中的内爆引爆波

Pushpender Kumar Gangwar, Rajesh Kumar Verma
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摘要

本文借助切斯特-奇斯内尔-惠瑟姆(CCW)理论,研究了在非均质介质自引力作用下,强球形内爆爆轰波在反应理想气体中的传播。我们认为起爆波最初是查普曼-朱盖特起爆波。最初将密度分布规律视为随距离递减的幂,从而推导出了前端后方爆轰速度的分析表达式以及其他流动变量。在不考虑超越扰动影响的情况下,对非维爆轰速度、压力和密度随传播距离的变化进行了数值计算。通过图表详细讨论了不同阿尔芬马赫数下密度参数的变化对爆轰前沿收敛的影响。最后发现,气体的密度参数和阿尔芬马赫数对反应理想气体中强球形爆轰前沿的传播具有重要作用,同时对所有后流变量具有引力效应。计算中使用了 MATLAB 软件。关键词自引力气体、强爆轰波、CCW 理论。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Imploding Detonation Waves in Self-gravitating Ideal Gas
In the present paper, the propagation of strong spherical imploding detonation waves in a reacting ideal gas under the effect of self-gravitation of the non-homogeneous medium has been investigated, by the help of Chester-Chisnell-Whitham (CCW) theory. It is considered that detonation wave is initially Chapman-Jouguet. Initial taking the density distribution law as power decreasing with distance, the analytical expressions for the detonation velocity just behind the front along with other flow variables are derived. Neglecting the effect of overtaking disturbances the variation of non-dimensional detonation velocity, the pressure and density with the propagation distance have been calculated numerically. The effect of change in density parameter at different Alfven Mach number on the convergence of detonation front have been discussed through graphs in details. Finally, it is found that density parameter and Alfven Mach number of gas have a significant role on propagation of strong spherical detonation front in reacting ideal gas with gravitation effect on all the post-flow variables. The software MATLAB have been used for computation of the problem. Keywords: Self-gravitating gas, Strong detonation waves, CCW theory.
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