SUMMARY
Direct collapsing black holes (DCBH) formed shortly after the Big Bang, potentially weighing millions of solar masses just 1 billion years post-event. Unlike traditional stellar black holes, which are limited by stellar evolution models, DCBHs are not mass constrained and can grow significantly through accretion and mergers. Their formation is influenced by the initial density fluctuations in the early universe, which were much greater than present conditions, allowing for the rapid accumulation of mass.
PREREQUISITES
- Understanding of direct collapsing black holes (DCBH)
- Knowledge of black hole formation mechanisms
- Familiarity with the Big Bang theory
- Concepts of density fluctuations in cosmology
NEXT STEPS
- Research the mechanisms of black hole accretion and mergers
- Study the implications of density fluctuations in the early universe
- Explore the differences between stellar black holes and direct collapsing black holes
- Investigate the role of the early universe's density in cosmic structure formation
USEFUL FOR
Astronomers, astrophysicists, and cosmologists interested in black hole formation and the early universe's conditions.