氢燃烧的非平衡热力学理论研究

Study of Hydrogen Burning Inside the Stars by Non—equilibrium Thermodynamics Theory

剧烈进行着热核反应的恒星是一个远离平衡态的开放系统。本文考虑到对流和扩散的因素,研究了氢燃烧的结构稳定性。

A star is an open system which is far away from thermodynamic equilibrium state. In view of the fact that the hydrogen burning inside the stars are very strong,we introduce the effects of convection and diffusion in the fumdamental equations. The structure stability of the hydrogen burning inside the star is studied and the results are obtained.