accdd
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Is it possible that galaxies are spinning faster than expected due to a particular configuration of the moving mass and not due to dark matter?
The discussion revolves around the dynamics of galaxy rotation, specifically questioning whether the observed faster spinning of galaxies can be attributed to configurations of visible mass rather than dark matter. The scope includes theoretical considerations and challenges to existing models of galaxy rotation curves.
Participants do not reach a consensus, as there are multiple competing views regarding the role of dark matter and alternative explanations for galaxy rotation. The discussion remains unresolved with ongoing debate about the validity of different models.
The discussion highlights limitations in understanding the gravitational effects of different mass configurations and the assumptions underlying current models of galaxy rotation. There are unresolved questions about the applicability of GR in this context.
No.accdd said:Is it possible that galaxies are spinning faster than expected due to a particular configuration of the moving mass and not due to dark matter?
Well, you could put rocket engines on all the stars.Nugatory said:No.
I thought Deur's idea was about GR effects of non-spherical configurations of matter, not about GR effects of rotating matter. His basic idea, as I understand it, is that the GR effects of a flat disk are significantly different from those of a sphere, and the standard method of calculating galaxy rotation curves is basically assuming that they're not, and using the simpler calculations for a sphere.Ibix said:Deur's idea that we've failed to properly account for the GR effects of rotating matter
You're more likely to be right than I am. Either way, he's explaining galaxy rotation curves using the visible matter and vanilla GR so he doesn't need dark matter. (Or so he says, anyway.)PeterDonis said:I thought Deur's idea was about GR effects of non-spherical configurations of matter, not about GR effects of rotating matter. His basic idea, as I understand it, is that the GR effects of a flat disk are significantly different from those of a sphere, and the standard method of calculating galaxy rotation curves is basically assuming that they're not, and using the simpler calculations for a sphere.
Yes, that's correct. But since the topic of this thread is particularly the effects of rotation, I don't think Deur's proposal is relevant to this particular thread.Ibix said:Either way, he's explaining galaxy rotation curves using the visible matter and vanilla GR so he doesn't need dark matter. (Or so he says, anyway.)