SUMMARY
Black holes can indeed combine to form larger black holes, with no known upper mass limit for their formation. The merging process does not involve "sucking" but rather the gravitational attraction between them. When two black holes merge, the resulting black hole has slightly less mass than the sum of the original black holes due to energy loss from gravitational waves. The total mass of the universe serves as a theoretical upper limit for black hole mass accumulation.
PREREQUISITES
- Understanding of general relativity and gravitational waves
- Familiarity with black hole formation and properties
- Knowledge of relativistic physics, particularly at high velocities
- Concept of spacetime and its implications in astrophysics
NEXT STEPS
- Research gravitational wave detection and its significance in black hole mergers
- Explore the concept of supermassive black holes and their formation in galaxies
- Study the implications of the Big Crunch theory in cosmology
- Investigate the role of relativistic effects in high-speed astrophysical phenomena
USEFUL FOR
Astronomers, astrophysicists, and students of physics interested in black hole dynamics and cosmological theories.