Undergrad Meaning of the distance between galactic objects in GR

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SUMMARY

The discussion focuses on the distance of Sagittarius A* (Sgr A*) from Earth, estimated at 26,996±29 light years, within the framework of General Relativity (GR). It highlights the inadequacy of the FLRW model for galactic scales, emphasizing that the weak field approximation provides a more accurate description of spacetime in this context. The conversation clarifies that the galactic rest frame is an irrotational frame where the galaxy's center of mass is at rest, and constituents of the galaxy move in approximately circular orbits around it.

PREREQUISITES
  • Understanding of General Relativity (GR)
  • Friedmann-Lemaître-Robertson-Walker (FLRW) model
  • Weak field approximation in GR
  • Concept of galactic center of mass (COM)
NEXT STEPS
  • Explore the implications of the weak field approximation in General Relativity
  • Study the dynamics of galaxies using the irrotational frame concept
  • Investigate the limitations of the FLRW model at galactic scales
  • Learn about the metric tensor in the context of spacetime manifolds
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Astronomers, physicists, and students of cosmology interested in the application of General Relativity to galactic structures and distances.

cianfa72
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TL;DR
About the meaning of the distance between galactic objects in the Universe in the context of GR
Hi, I was thinking about the claim that for instance Sagittarius A* (Sgr A*) black hole is a at 26996±29 light years from the Earth from a GR point of view.

Assuming a FLRW model for the Universe, maybe the above meaning is that at a given cosmological time ##t## (the "present" time) the proper distance between the Earth and Sgr A* evaluated on the spacelike hypersurface of constant cosmological time ##t## is actually 26996±29 light year.

Does it make sense ?
 
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The FLRW model is not a good model at the galactic scale as the galaxy is a gravitationally bound system. Instead, the spacetime on galactic level is pretty well described (apart from locally near extreme objects like black holes) by the weak field approximation. Sgr A* being some 27000 ly away is the corresponding distance in the galactic rest frame.
 
Orodruin said:
Instead, the spacetime on galactic level is pretty well described (apart from locally near extreme objects like black holes) by the weak field approximation. Sgr A* being some 27000 ly away is the corresponding distance in the galactic rest frame.
Does the weak field approximation give rise to a metric tensor on spacetime as a manifold ?

Edit: is the galactic rest frame the spacetime coordinate chart in which on average the galaxy's constituents are "at rest" -- i.e. have timelike worldlines with constant spatial coordinates?
 
Last edited:
cianfa72 said:
Does the weak field approximation give rise to a metric tensor on spacetime as a manifold ?

Yes.


cianfa72 said:
Edit: is the galactic rest frame the spacetime coordinate chart in which on average the galaxy's constituents are "at rest" -- i.e. have timelike worldlines with constant spatial coordinates?
No. It is the irrotational frame where the galaxy com is at rest.
 
Orodruin said:
No. It is the irrotational frame where the galaxy com is at rest.
Could you be more specific ? As far as I can understand, it is the coordinate chart in which the galaxy's COM (Center of Mass) is "at rest" -- i.e. its timelike worldline has constant spatial coordinates in that chart (only varying timelike coordinate time ##t##).

What does it mean it is an irrotational frame/coordinate chart ? Thanks.
 
cianfa72 said:
What does it mean it is an irrotational frame/coordinate chart ?
Does not rotate with the galaxy.
 
Orodruin said:
Does not rotate with the galaxy.
Sorry, I don't grasp the point. Do the galaxy's constituents rotate in that irrotational chart (i.e. their timelike worldlines parametrized by the coordinate time ##t## rotate in that chart) ?
 
cianfa72 said:
Do the galaxy's constituents rotate in that irrotational chart
Yes, they move around in approximately circular orbits.
 
Orodruin said:
Yes, they move around in approximately circular orbits.
Ah ok, that means galaxy's constituents paths (parametrized by the coordinate time ##t##) as described in the irrotational chart move like circular orbits around the galaxy's COM.
 
Last edited:
  • #10
Well, approximately circular. There are lots of local variations to that, but in general yes.
 

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