SUMMARY
The discussion centers on the existence of Schwarzschild black holes, with participants expressing skepticism about their non-rotating nature. It is established that all known black holes are likely Kerr black holes, which possess angular momentum. The conversation highlights that even a single photon can impart angular momentum to a black hole, making non-rotating black holes extremely unlikely. Additionally, the spin of black holes, particularly the measurement of the spin of the supermassive black hole in NGC 1365, is discussed, emphasizing the complexities of defining spin in the context of general relativity.
PREREQUISITES
- Understanding of Kerr black holes and their properties
- Familiarity with concepts of angular momentum in astrophysics
- Basic knowledge of general relativity and singularities
- Awareness of observational techniques for measuring black hole spin
NEXT STEPS
- Research the properties and implications of Kerr black holes
- Study the methods for measuring black hole spin, particularly frame dragging
- Explore the relationship between black hole spin and the dynamics of accretion disks
- Investigate the mathematical models used to describe black hole singularities
USEFUL FOR
Astronomers, astrophysicists, and students of theoretical physics who are interested in black hole mechanics, particularly the dynamics of rotating black holes and their observational characteristics.