SUMMARY
Quasars are powered by supermassive black holes (SMBHs) at the centers of galaxies, surrounded by active accretion disks composed primarily of hydrogen and helium. These disks generate significant electromagnetic (EM) radiation due to gravitational compression and friction as matter falls into the black hole. The accretion process is highly efficient, converting up to 10% of the mass into energy, making quasars some of the brightest objects in the universe. Over time, SMBHs may exhaust their fuel supply and enter a dormant state, potentially reactivated by galactic mergers.
PREREQUISITES
- Understanding of supermassive black holes (SMBHs)
- Knowledge of accretion disk dynamics
- Familiarity with electromagnetic radiation principles
- Basic concepts of mass-energy equivalence
NEXT STEPS
- Research the mechanics of accretion disks in astrophysics
- Study the lifecycle of supermassive black holes
- Explore the relationship between quasars and galaxy evolution
- Investigate the implications of Hawking radiation on black hole longevity
USEFUL FOR
Astronomers, astrophysics students, and anyone interested in the dynamics of black holes and their role in galaxy formation and evolution.