Как да изчислим Chandrasekhar Limit
Какво е Chandrasekhar Limit?
Chandrasekhar limit (~1.4 solar masses) is maximum mass white dwarf can support against gravitational collapse via electron degeneracy pressure.
Ръководство стъпка по стъпка
- 1Input white dwarf mass
- 2Compare to Chandrasekhar limit
- 3Determine stability or collapse fate
Worked Examples
Вход
WD mass 1.2 M☉
Резултат
Below limit, stable
Above limit → neutron star
Common Mistakes to Avoid
- ✕Confusing with Tolman-Oppenheimer-Volkoff limit
- ✕Assuming constant value (varies slightly)
Frequently Asked Questions
What happens above limit?
Electron degeneracy fails; collapse to neutron star or black hole.
Готови ли сте да изчислите? Опитайте безплатния калкулатор Chandrasekhar Limit
Опитайте сами →