Discussion Overview
The discussion revolves around the characteristics of rotating (Kerr) and non-rotating (Schwarzschild) black holes, focusing on the factors that determine a black hole's rotation and the implications of angular momentum as described by the No Hair theorem.
Discussion Character
- Exploratory
- Technical explanation
- Debate/contested
Main Points Raised
- One participant questions what determines whether a black hole will rotate or not, and seeks to understand the implications of zero angular momentum.
- Another participant states that a Kerr black hole forms from a star or system of stars with nonzero angular momentum.
- It is noted that in the limit of zero angular momentum, the Kerr solution becomes the Schwarzschild solution, indicating that a non-rotating Kerr black hole is equivalent to a Schwarzschild black hole.
- A participant asserts that real black holes effectively always rotate, suggesting that the likelihood of a black hole having zero angular momentum is extremely low.
- It is mentioned that while non-rotating black holes are simpler and lack features like the ergosphere or jets, they serve as useful theoretical constructs.
- Another participant explains that angular momentum is conserved, implying that if the progenitor star had angular momentum, the resulting black hole will also rotate.
Areas of Agreement / Disagreement
Participants express differing views on the prevalence of non-rotating black holes, with some suggesting they are theoretical constructs while others emphasize the rarity of such black holes in reality. The discussion remains unresolved regarding the implications of angular momentum and the conditions under which a black hole might not rotate.
Contextual Notes
Participants highlight the complexity of rotating black holes compared to non-rotating ones, but do not resolve the assumptions about the conditions necessary for a black hole to have zero angular momentum.