Cum se calculează Chandrasekhar Limit
Ce este Chandrasekhar Limit?
Chandrasekhar limit (~1.4 solar masses) is maximum mass white dwarf can support against gravitational collapse via electron degeneracy pressure.
Ghid pas cu pas
- 1Input white dwarf mass
- 2Compare to Chandrasekhar limit
- 3Determine stability or collapse fate
Exemple rezolvate
Intrare
WD mass 1.2 M☉
Rezultat
Below limit, stable
Above limit → neutron star
Greșeli frecvente de evitat
- ✕Confusing with Tolman-Oppenheimer-Volkoff limit
- ✕Assuming constant value (varies slightly)
Întrebări frecvente
What happens above limit?
Electron degeneracy fails; collapse to neutron star or black hole.
Ești gata să calculezi? Încercați calculatorul gratuit Chandrasekhar Limit
Încercați singur →