Discussion Overview
The discussion revolves around the concept of a smaller black hole potentially existing within the event horizon of a larger black hole, exploring theoretical implications and scenarios. Participants examine the nature of black holes, event horizons, and gravitational interactions, with a focus on both theoretical and conceptual aspects.
Discussion Character
- Exploratory
- Debate/contested
- Conceptual clarification
- Technical explanation
Main Points Raised
- Some participants propose that a smaller black hole could orbit a larger black hole, questioning the implications of such a scenario.
- Others argue that as black holes approach each other, their orbits become nonlinear, leading to merging rather than stable orbits.
- A participant suggests that a swarm of stars could exist within its own Schwarzschild radius, potentially allowing for a black hole to be part of this configuration.
- There is a discussion about the definitions of event horizons, with some participants noting that the standard definition may not apply to inner bodies within a black hole.
- Some participants assert that concepts of time and space lose meaning inside a black hole's event horizon, while others challenge this view, suggesting that they remain meaningful except near the singularity.
- One participant raises the issue of how a black hole could be perceived from within another black hole's event horizon, introducing the need for different coordinate charts.
- There are references to gravitational time dilation and the effects of mass both inside and outside a black hole, with implications for the nature of black holes in such configurations.
- Some participants express caution regarding assumptions about the creation of a common event horizon from multiple black holes, noting a lack of supporting theorems.
Areas of Agreement / Disagreement
Participants do not reach a consensus; multiple competing views remain regarding the nature of black holes, event horizons, and the implications of one black hole existing within another.
Contextual Notes
Discussions include limitations related to definitions of event horizons, the stability of configurations involving multiple black holes or stars, and the applicability of Schwarzschild solutions to non-empty black holes.