Discussion Overview
The discussion revolves around the existence of orbiting black holes, specifically focusing on stellar black holes orbiting supermassive black holes and the dynamics of black hole pairs orbiting each other. It explores theoretical implications and observational evidence related to these scenarios.
Discussion Character
- Exploratory
- Technical explanation
- Debate/contested
Main Points Raised
- Some participants inquire about evidence for stellar black holes orbiting supermassive black holes in galaxy centers.
- Others propose that if two black holes come close enough for their event horizons to touch, they would merge into a larger black hole, potentially emitting gravitational waves.
- Several participants mention strong candidates for galaxies with two supermassive black holes orbiting each other, suggesting they will eventually merge and emit gravitational waves.
- One participant raises questions about the nature of the area near the center of mass of two orbiting black holes, speculating on tidal forces and the turbulence of spacetime in that region.
Areas of Agreement / Disagreement
Participants generally agree on the potential for black holes to merge and emit gravitational waves, but the discussion includes various speculative aspects regarding the nature of the spacetime around orbiting black holes and the specifics of their interactions, indicating unresolved questions and differing viewpoints.
Contextual Notes
Participants express assumptions about the conditions under which black holes might interact, such as the spacing between them and the effects of their mass on tidal forces. There are unresolved questions about the observational evidence for these scenarios and the exact nature of the spacetime dynamics involved.