Jinsi ya kukokotoa Chandrasekhar Limit
Chandrasekhar Limit ni nini?
Chandrasekhar limit (~1.4 solar masses) is maximum mass white dwarf can support against gravitational collapse via electron degeneracy pressure.
Mwongozo wa Hatua kwa Hatua
- 1Input white dwarf mass
- 2Compare to Chandrasekhar limit
- 3Determine stability or collapse fate
Mifano Iliyotatuliwa
Ingizo
WD mass 1.2 M☉
Matokeo
Below limit, stable
Above limit → neutron star
Makosa ya Kawaida ya Kuepuka
- ✕Confusing with Tolman-Oppenheimer-Volkoff limit
- ✕Assuming constant value (varies slightly)
Maswali yanayoulizwa mara kwa mara
What happens above limit?
Electron degeneracy fails; collapse to neutron star or black hole.
Je, uko tayari kukokotoa? Jaribu Kikokotoo kisicholipishwa cha Chandrasekhar Limit
Jaribu mwenyewe →