SUMMARY
The discussion centers on the examination of the spectrum of gravitationally lensed light, particularly focusing on potential red or blue shifts observed in different parts of an Einstein ring. Participants clarify that, according to General Relativity (GTR), light bending does not depend on frequency. However, Rudi Van Nieuwenhove raises the possibility of frequency shifts due to strong frame-dragging effects around massive rotating bodies, such as black holes or galaxies. The conversation references Chandrasekhar's "Mathematical Theory of Black Holes" for further exploration of these concepts.
PREREQUISITES
- Understanding of General Relativity (GTR)
- Familiarity with gravitational lensing concepts
- Knowledge of Einstein rings and their characteristics
- Basic principles of frame dragging in astrophysics
NEXT STEPS
- Study the effects of frame dragging in rotating black holes
- Research the mathematical framework in Chandrasekhar's "Mathematical Theory of Black Holes"
- Examine observational techniques for measuring red and blue shifts in astrophysics
- Explore the implications of gravitational lensing on cosmological observations
USEFUL FOR
Astronomers, astrophysicists, and students interested in gravitational lensing, black hole physics, and the implications of General Relativity on light propagation.