Discussion Overview
The discussion revolves around the mass of black holes, particularly focusing on where the mass is located, the implications of supernovae and hypernovae on black hole formation, and the nature of singularities. Participants explore theoretical concepts, physical implications, and the challenges of understanding black hole interiors.
Discussion Character
- Exploratory
- Technical explanation
- Conceptual clarification
- Debate/contested
Main Points Raised
- One participant questions how a black hole can have significant mass if much of it is ejected during supernova events, suggesting uncertainty about the mass's location.
- Another participant states that while mass is concentrated in a small region, it is unlikely to be a singularity of zero size, proposing that unknown physics may prevent complete collapse.
- A different viewpoint introduces the Hayward metric as a potential model that avoids singularities, suggesting that some mass may exist at a non-zero size.
- Several participants discuss whether the mass of a black hole is located at the singularity or distributed throughout the region inside the event horizon, with some asserting that most of this region is vacuum.
- One participant clarifies that outside the event horizon, the mass behaves like a point source, similar to other celestial objects.
- Another participant emphasizes that the event horizon defines the observable size of a black hole, and its interior remains speculative, with the Planck density being a reasonable consideration.
- One participant explains that the core of a star, which is denser than the outer layers, is what ultimately contributes to the black hole's mass after a supernova, referencing the Chandrasekhar Limit.
Areas of Agreement / Disagreement
Participants express multiple competing views regarding the nature of mass in black holes and the implications of singularities. The discussion remains unresolved, with no consensus on the exact location or nature of mass within black holes.
Contextual Notes
There are limitations in the discussion regarding assumptions about the nature of singularities, the definitions of mass concentration, and the speculative nature of black hole interiors. Mathematical steps and physical implications are not fully resolved.