“Chandrasekhar limit”的概念、定义、习题解题方法及翻译-物理辞典

单词	Chandrasekhar limit
释义	Chandrasekhar limit The maximum possible mass of a star that is prevented from collapsing under its own gravity by the degeneracy pressure of either electrons (a white dwarf) or neutrons (a neutron star). For white dwarfs the Chandrasekhar mass is about 1.4 times the mass of the sun. For neutron stars its value is less precisely known because of uncertainties regarding the equation of state of neutron matter, but it is generally taken to be in the range of 1.5 to 3 (and almost certainly no more than 5) times the mass of the sun. It is named after the Indian-born US astrophysicist Subrahmanyan Chandrasekhar (1910–95)
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物理辞典收录了3346条物理词条，基本涵盖了常用物理知识及物理英语单词词组的翻译及用法，是物理学习的有利工具。