SUMMARY
The discussion centers on the fate of matter that falls into a black hole, concluding that current understanding is limited. General relativity predicts that matter is compressed to a singularity, leading to infinite density, but this remains speculative due to the extreme conditions involved. The Einstein-Cartan theory offers alternative insights, yet consensus on quantum gravity is lacking. Notably, the Chandrasekhar Limit indicates that neutron degeneracy pressure cannot support stars exceeding approximately 1.4 solar masses, leading to black hole formation.
PREREQUISITES
- Understanding of General Relativity (GR)
- Familiarity with the concept of singularities
- Knowledge of neutron degeneracy pressure
- Basic principles of quantum gravity theories
NEXT STEPS
- Research the Einstein-Cartan theory and its implications for black hole physics
- Study the Chandrasekhar Limit and its role in stellar evolution
- Explore the 1990 paper by Poisson and Israel on the internal structure of black holes
- Investigate current theories of quantum gravity and their potential effects on black hole matter
USEFUL FOR
Astronomers, physicists, and students of theoretical physics seeking to deepen their understanding of black hole mechanics and the behavior of matter under extreme gravitational conditions.