Discussion Overview
The discussion centers around the potential influence of the spin of supermassive black holes (SMBHs) on the rotation of their host galaxies. Participants explore whether there is a direct or correlative effect between the two, considering various formation scenarios for both SMBHs and galaxies.
Discussion Character
- Debate/contested
- Exploratory
- Technical explanation
Main Points Raised
- Some participants propose that the spin of a supermassive black hole may not exert a force on the galaxy, but they could rotate in the same direction due to their formation from the same rotating mass.
- Others argue that supermassive black holes typically form through mergers, which complicates the relationship between their spin and the galaxy's rotation.
- It is suggested that if a supermassive black hole forms after the galaxy has developed its spin, the black hole's spin may not influence the galaxy's rotation.
- Some participants express skepticism about the significance of black hole spin on galactic rotation, mentioning local frame dragging effects as potentially negligible on galactic scales.
- There is a discussion about whether all galaxies require a supermassive black hole at their center, with some noting that while many seem to have them, it is not definitively proven.
- One participant mentions that the formation of supermassive black holes might involve the coalescence of a central mass of stars rather than direct collapse, raising questions about the mechanisms involved.
- Another viewpoint suggests that the dynamics of a galaxy could be influenced by dark matter rather than the spin of the central black hole.
- Several participants express uncertainty about the physical realizability of different formation scenarios for supermassive black holes.
Areas of Agreement / Disagreement
Participants do not reach a consensus on the relationship between the spin of supermassive black holes and the rotation of galaxies. Multiple competing views remain, with ongoing debate about the mechanisms of formation and influence.
Contextual Notes
Limitations include unresolved assumptions about the formation processes of supermassive black holes and galaxies, as well as the dependence on definitions of spin and rotation in different contexts.