SUMMARY
Black holes form from the gravitational collapse of massive stars, leading to a supernova explosion. During this process, matter becomes so dense that internal pressure cannot prevent further collapse, potentially resulting in a singularity. Observers cannot witness the formation of a black hole due to gravitational time dilation, which causes infalling material to appear to slow and fade away as it approaches the event horizon. Current understanding of the fate of neutrons and quarks during this collapse remains speculative, with no verified equations or physical descriptions available.
PREREQUISITES
- Understanding of gravitational collapse and supernovae
- Familiarity with concepts of degeneracy pressure and singularities
- Basic knowledge of astrophysics and black hole formation theories
- Awareness of gravitational time dilation effects
NEXT STEPS
- Research the role of degeneracy pressure in stellar collapse
- Explore Kip Thorne's theories on black holes and singularities
- Study the implications of gravitational time dilation on black hole observation
- Investigate current theories in quantum gravity and string theory
USEFUL FOR
Astronomy enthusiasts, astrophysicists, and students studying black hole formation and the underlying physics of gravitational collapse.