Chandrasekhar limit

Chandrasekhar Limit Based on the Model of Relativistic Degenerate Fermi Gas

基于相对论简并费米气体模型的Chandrasekhar极限

Theory predicts that a white dwarf star will explode when infalling matter from a companion star increases the mass of the white dwarf beyond a critical mass limit , known as the Chandrasekhar limit .

理论预言，当来自伴星的物质让白矮星的质量增加到了临界质量极限即钱德拉塞卡极限时，白矮星就会爆发。

Using degenerate Fermi statistics theory and considering the relativistic effect of electronic move - ment , this paper derives limited mass of White Dwarf Stars-Chandrasekhar limit , and then discusses the importance of Chandrasekhar limit in the stellar evolution process .

利用简并费米统计理论，并考虑到电子运动的相对论效应，求出白矮星的极限质量&Chan-drasekhar极限质量，并进一步讨论了这一极限质量在恒星演化过程中的意义。