Discussion Overview
The discussion revolves around the question of why black holes do not become stars again despite consuming hydrogen and having sufficient gravitational pressure. Participants explore the processes of fusion, the nature of black holes, and the conditions under which stars form, while addressing the complexities involved in these phenomena.
Discussion Character
- Exploratory
- Technical explanation
- Conceptual clarification
- Debate/contested
Main Points Raised
- Some participants propose that fusion occurs within the event horizon of a black hole, but it is unclear what happens at the singularity.
- One participant explains that the core of a neutron star, which is similar to a black hole, cannot undergo fusion due to the absence of atomic nuclei.
- Another participant describes the fusion process in normal stars, emphasizing that once a black hole forms, the event horizon prevents any fusion from occurring within it.
- Some participants suggest that the immense pressure inside a black hole surpasses neutron-degenerate pressure, complicating the conditions for fusion.
- There is mention of fusion occurring in the accretion disk surrounding a black hole, but it is noted that nothing escapes from the black hole itself.
- One participant raises the idea that energy may leave a black hole through quantum effects, but this does not equate to information escaping.
Areas of Agreement / Disagreement
Participants express various viewpoints on the nature of fusion in relation to black holes, with no consensus reached on whether fusion can occur within a black hole or the implications of such processes.
Contextual Notes
There are limitations regarding the understanding of conditions inside a black hole, particularly past the event horizon, and the nature of fusion under extreme pressures is not fully resolved.