SUMMARY
Time does not stop at the event horizon of a black hole from the perspective of an observer. A massive object collapses into a black hole in a finite time as perceived by an observer falling with the collapse. An observer at a distance will see the collapsing star become increasingly redshifted until it is no longer visible, but this does not negate the existence of the black hole. The formation of a black hole is a definitive event in spacetime, independent of the observer's perspective.
PREREQUISITES
- Understanding of general relativity and spacetime geometry
- Familiarity with black hole formation and event horizons
- Knowledge of redshift and its implications in astrophysics
- Basic concepts of gravitational binding in binary systems
NEXT STEPS
- Research the implications of general relativity on black hole formation
- Study the concept of redshift and its observational effects on distant objects
- Explore the characteristics of accretion disks around black holes
- Learn about the global spacetime geometry and its relation to black holes
USEFUL FOR
Astronomers, astrophysicists, and students of physics interested in black hole dynamics and observational cosmology.