Discussion Overview
The discussion revolves around the effects of galactic rotation on the energy-momentum tensor and its implications for understanding galaxy dynamics, particularly in relation to dark matter. Participants explore the relevance of general relativity (GR) versus Newtonian models in explaining the rotation curves of galaxies.
Discussion Character
- Exploratory
- Technical explanation
- Debate/contested
Main Points Raised
- Some participants propose that the global rotation of galaxies could influence the energy-momentum tensor, potentially affecting space-time and star movements, similar to the Kerr model for black holes.
- Others argue that in modeling galaxies, GR effects are typically negligible, leading to the use of Newtonian gravity, which simplifies the analysis.
- There is a question about whether the angular momentum of the internal mass should be included to account for frame dragging effects.
- Some participants suggest that GR might eliminate the need for dark matter to explain the velocities of stars in the outer regions of galaxies, citing a paper that supports this view.
- A later reply questions the validity of the claim that GR alone can account for galaxy rotation curves without dark matter, indicating that this remains an open question in the field.
Areas of Agreement / Disagreement
Participants express differing views on the applicability of GR versus Newtonian models in explaining galaxy dynamics. There is no consensus on whether GR can fully account for observed phenomena without invoking dark matter, and the discussion remains unresolved.
Contextual Notes
Limitations include the dependence on the assumptions made in modeling galaxies, the complexity added by incorporating GR effects, and the unresolved nature of claims regarding the sufficiency of GR to explain galaxy rotation without dark matter.