What stellar remnant is stabilized primarily by electron degeneracy pressure?
Answer
White dwarf
For stars less massive than certain thresholds, the remnant core stabilizes as a white dwarf, supported by the incredibly strong force of electron degeneracy pressure.
#Videos
Why Don't Main Sequence Stars Explode Or Collapse? - YouTube
Related Questions
What is the key concept governing a star's stable existence against gravitational collapse?In main-sequence stars like the Sun, what generates the necessary outward pressure to counteract gravity?What process occurs in the Sun's core at about 15 million degrees Celsius?How does a main-sequence star maintain stability if the core momentarily cools?For stars similar to or less massive than the Sun, what non-thermal mechanism halts core collapse after hydrogen fuel runs out?Which quantum mechanical principle underlies the concept of degeneracy pressure?What stellar remnant is stabilized primarily by electron degeneracy pressure?What pressure supports a neutron star formed after gravity overcomes electron degeneracy pressure?What is the approximate mass limit defining stable white dwarfs supported by electron degeneracy?What ultimate condition leads to the formation of a black hole?How does degeneracy pressure differ from thermal pressure based on temperature?