What quantum mechanical force prevents a white dwarf core from collapsing further than the Chandrasekhar limit?
Answer
Electron degeneracy pressure
Electron degeneracy pressure is a quantum mechanical effect where electrons resist occupying the same quantum state, providing the necessary outward support for a white dwarf.
Related Questions
What final stellar remnant will our Sun become?What quantum mechanical force prevents a white dwarf core from collapsing further than the Chandrasekhar limit?What is the approximate maximum mass limit for a stable white dwarf?Which pressure supports a neutron star against further gravitational collapse?What is the approximate upper mass limit for a neutron star, known as the TOV limit?What is the general requirement for a star's *initial* mass to potentially form a black hole remnant?What occurs if the remnant core following a supernova weighs more than the TOV limit?What term describes the challenging observational region for compact objects with masses between about 2 and 5 solar masses?According to current understanding, why can our Sun never become a black hole?What is the typical mass range for Supermassive Black Holes (SMBHs)?