Galactic Rotation and Energy-Momentum Tensor

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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.

Christian Thom
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TL;DR
Is the momentum part of the energy/momentum tensor taken into account in the modelling of the movements of the stars in galaxies ?
Galaxies are very large rotating bodies, so it seems that, as with the Kerr model for black holes, there could be an effect of this global rotation on the energy momentum tensor in the more dense regions of the galaxy that could in turn affect the space-time in the vicinity of the object and so the movements of the stars, with maybe an impact on the evaluation of the dark matter quantity.
 
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Christian Thom said:
as with the Kerr model for black holes, there could be an effect of this global rotation on the energy momentum tensor
Kerr black holes are vacuum solutions, so the stress-energy tensor is zero everywhere.

In modeling galaxies, GR effects are typically negligible so a Newtonian model of gravity is used.
 
Thank you.
 
Does the angular momentum of the internal mass need to be accounted for so the frame dragging is included?
 
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richardgobeli said:
Does the angular momentum of the internal mass need to be accounted for so the frame dragging is included?
Depends how precise you want to be. The usual modelling of galaxies is Newtonian because GR effects are negligible and adding them in simply increases the complexity of the model without making any measurable change to the output. But if you wanted to make the effort, you would need to include the rotation of the galactic disc if you wanted to see frame dragging effects.
 
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GR can be used to make the rotating galaxy not need dark matter to make the velocities constant in the outer rim of the galaxy. Newtonian gravity does not account for the local frame dragging of the local stars to the test star. Here is a paper that shows that dark matter is not needed when GR is used and the angular momentum of the galactic disk is used. https://arxiv.org/abs/2207.04279 titled

General Relativity versus Dark Matter for rotating galaxies​

Even when the stress-energy tensor is zero, the metric of the rotating galaxy contains the angular momentum of the rotating galaxy which does pull the rim stars along at a higher velocity rate than Newtonian gravity allows.
 
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richardgobeli said:
Here is a paper that shows that dark matter is not needed when GR is used and the angular momentum of the galactic disk is used. https://arxiv.org/abs/2207.04279 titled

General Relativity versus Dark Matter for rotating galaxies​

We have had a previous thread on this paper:

https://www.physicsforums.com/threa...ng-gr-explains-dark-matter-phenomena.1016800/

The short version is that it is not clear that the claim of this paper, that the GR frame dragging effect due to rotation is sufficient to account for galaxy rotation curves without dark matter, is correct; it's still an open question. It's a very interesting proposal but it can't be taken as mainstream accepted science, at least not at this point.
 
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