Discussion Overview
The discussion centers around the time it takes for a black hole to accumulate mass, specifically addressing the scenario of a black hole gaining seven billion solar masses. Participants explore theoretical aspects, observational evidence, and the implications of black hole formation in the context of the universe's age and material availability.
Discussion Character
- Exploratory
- Debate/contested
- Technical explanation
- Conceptual clarification
Main Points Raised
- Some participants suggest that black holes accumulate matter over long periods, with significant mass gain occurring only under certain conditions, such as starting with a massive star.
- Others argue that the formation of supermassive black holes may have occurred rapidly in the early universe, potentially from primordial gas clouds rather than from stellar evolution.
- There is a discussion about the probability of forming stellar black holes, with some participants noting that while massive stars are rare, they are still capable of forming black holes through supernova events.
- Questions are raised regarding the mass thresholds for black hole formation and whether all black holes must originate from stars of a certain mass.
- Some participants inquire about the effects of time dilation on the mass accumulation of black holes, particularly in relation to accretion processes and the perception of time by distant observers.
- Concerns are expressed about the availability of material for black holes to accrete, suggesting that location within a galaxy may influence mass gain rates.
- Participants note the mystery surrounding the existence of quasars and supermassive black holes in the early universe, highlighting the challenges in explaining their rapid formation.
Areas of Agreement / Disagreement
Participants express a range of views on the mechanisms and timelines for black hole mass accumulation, with no consensus reached on the specifics of formation processes or the implications of time dilation. The discussion remains unresolved regarding the exact conditions necessary for black hole growth and the probabilities associated with different mass ranges.
Contextual Notes
Limitations include uncertainties about the initial conditions for black hole formation, the dependence on definitions of mass thresholds, and unresolved questions regarding the mechanisms of accretion and time dilation effects.