Discussion Overview
The discussion revolves around the potential maximum size a black hole could achieve if it were continuously fed with matter, exploring theoretical limits and the dynamics involved. Participants consider various factors influencing black hole growth, including angular momentum, surrounding material, and the nature of gravitational interactions.
Discussion Character
- Exploratory
- Debate/contested
- Conceptual clarification
- Technical explanation
Main Points Raised
- Some participants propose that a black hole would simply grow in mass and size without losing its black hole characteristics, while others question if there are limits to this growth based on surrounding material availability.
- One participant mentions a theoretical limit of 50 billion solar masses, citing astronomers who suggest this limit arises from a black hole's ability to clear its vicinity of material.
- Another viewpoint suggests that controlled feeding with angular momentum could allow a black hole to exceed this limit by preventing the formation of an accretion disk.
- Some participants argue that the analogy of a black hole functioning like a vacuum cleaner is misleading, emphasizing that falling into a black hole is not as straightforward as it may seem.
- There is a discussion about the nature of the universe and whether it could exist at a size and density that avoids becoming a black hole, with references to the universe's shape and density.
- Questions are raised about the potential for very large diffuse gas clouds to exist within their Schwarzschild radius and what limits their size, suggesting that larger clouds could theoretically exist.
Areas of Agreement / Disagreement
Participants express a range of views on the limits of black hole growth, with no consensus reached. Some agree on the idea of limits based on material availability, while others propose alternative scenarios that challenge this notion.
Contextual Notes
Limitations in the discussion include assumptions about the nature of black hole feeding, the dynamics of gravitational interactions, and the speculative nature of controlled feeding scenarios. The conversation also touches on the complexities of black hole characteristics compared to other massive objects.