SUMMARY
When two black holes collide, they merge to form a new black hole with an event horizon area that is equal to or larger than the sum of the original black holes' event horizons, as explained by Stephen Hawking's work. Black holes possess finite mass, contrary to the misconception that they have infinite mass, and their gravitational pull is strong enough to prevent light from escaping once it crosses the event horizon. The Schwarzschild Radius is the key concept for calculating the event horizon, which involves principles from General Relativity and differential geometry.
PREREQUISITES
- Understanding of General Relativity
- Familiarity with the concept of event horizons
- Knowledge of the Schwarzschild Radius
- Basic principles of differential geometry
NEXT STEPS
- Research the implications of Stephen Hawking's theories on black holes
- Study the calculations involved in determining the Schwarzschild Radius
- Explore video simulations of black hole collisions and mergers
- Investigate the theoretical existence of Tachyons and their properties
USEFUL FOR
Astronomers, physicists, students of astrophysics, and anyone interested in the dynamics of black holes and gravitational theories.