SUMMARY
A photon can theoretically orbit a black hole in a region known as the photon sphere, which is located at a radius of 3M for non-rotating black holes, where M is the mass of the black hole. However, this orbit is unstable and will not persist indefinitely due to the effects of gravity, which become increasingly strong as the photon approaches the event horizon (EH) at 2M. Once a photon crosses the EH, it cannot escape, and its trajectory is irrevocably altered. The discussion highlights the limitations of light's ability to maintain an orbit around a black hole and the implications of diffraction on its stability.
PREREQUISITES
- Understanding of black hole physics, specifically event horizons and photon spheres.
- Familiarity with general relativity concepts, including Kruskal–Szekeres coordinates.
- Knowledge of light behavior, particularly diffraction and its effects on photon trajectories.
- Basic mathematical skills for integrating equations related to light and black holes.
NEXT STEPS
- Research the properties of the photon sphere in both rotating and non-rotating black holes.
- Study the implications of Kruskal–Szekeres coordinates in black hole physics.
- Explore the mathematical equations governing light behavior near black holes, including integration techniques.
- Investigate the effects of tidal forces on light trajectories in strong gravitational fields.
USEFUL FOR
Astronomers, physicists, and students of astrophysics who are interested in the dynamics of light in extreme gravitational fields and the behavior of black holes.