SUMMARY
This discussion centers on the possibility of quantum entanglement between black holes and stars, particularly white dwarfs. Participants clarify that while black holes form from the gravitational collapse of large stars, there is no direct evidence of quantum entanglement between them. Observations from Gravitational Wave Observatories indicate that black holes merge, forming a single event horizon, rather than exhibiting a "tunnel closing" phenomenon. The conversation also highlights the behavior of stars near black holes, which are typically torn apart and contribute to an accretion disk rather than maintaining any entangled state.
PREREQUISITES
- Understanding of black hole formation and types, including stellar black holes.
- Familiarity with quantum entanglement principles in physics.
- Knowledge of gravitational waves and their significance in astrophysics.
- Awareness of accretion disks and their role in black hole dynamics.
NEXT STEPS
- Research the principles of quantum entanglement in astrophysical contexts.
- Explore the mechanics of black hole mergers as observed by LIGO and Virgo observatories.
- Study the formation and characteristics of accretion disks around black holes.
- Investigate the implications of gravitational wave detections on our understanding of black hole physics.
USEFUL FOR
Astronomers, physicists, and students interested in black hole dynamics, quantum mechanics, and the latest advancements in gravitational wave research.