如何计算Chandrasekhar Limit
learn.whatIsHeading
Chandrasekhar limit (~1.4 solar masses) is maximum mass white dwarf can support against gravitational collapse via electron degeneracy pressure.
分步指南
- 1Input white dwarf mass
- 2Compare to Chandrasekhar limit
- 3Determine stability or collapse fate
例题解析
输入
WD mass 1.2 M☉
结果
Below limit, stable
Above limit → neutron star
常见错误注意事项
- ✕Confusing with Tolman-Oppenheimer-Volkoff limit
- ✕Assuming constant value (varies slightly)
常见问题
What happens above limit?
Electron degeneracy fails; collapse to neutron star or black hole.
准备好计算了吗？尝试免费的 Chandrasekhar Limit 计算器
自己尝试一下 →