Understanding Homogeneity & Isotropy in FRW Metric

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SUMMARY

The discussion centers on the concepts of homogeneity and isotropy within the Friedmann-Robertson-Walker (FRW) metric. It establishes that the metric can be expressed as ##ds^{2}=-dt^{2}+a^{2}(t)\gamma_{ij}(u)du^{i}du^{j}##, where ##\gamma_{ij}## represents the metric of a spacelike slice at a constant time. Key points include that homogeneity is maintained when the scale factor ##a(t)## is appropriately incorporated, and isotropy allows for the elimination of cross-terms in the metric. The conversation emphasizes the importance of coordinate choice in understanding these properties.

PREREQUISITES
  • Understanding of Friedmann-Robertson-Walker (FRW) metric
  • Familiarity with concepts of homogeneity and isotropy in cosmology
  • Knowledge of spacetime metrics and their mathematical representations
  • Basic grasp of coordinate transformations in general relativity
NEXT STEPS
  • Study the derivation of the Friedmann-Robertson-Walker metric in detail
  • Explore the implications of coordinate choices on spacetime metrics
  • Learn about the role of scale factors in cosmological models
  • Investigate the mathematical properties of isotropic and homogeneous spaces
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Cosmologists, theoretical physicists, and students of general relativity seeking to deepen their understanding of the FRW metric and its implications for the structure of the universe.

binbagsss
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So in deriving the metric, the space-time can be foliated by homogenous and isotropic spacelike slices.

And the metric must take the form:

##ds^{2}=-dt^{2}+a^{2}(t)\gamma_{ij}(u)du^{i}du^{j}##,

where ## \gamma_{ij} ## is the metric of a spacelike slice at a constant t

QUESTION:
So I've read that:
1) Homogenity would be broken if the a(t) was taken outside the metric
2) By isotropicity there can be no cross-terms dtdx, dtdy, dtdz.

What I know:
homogenous means the same throughout - translationally invariant.
isotropic means the same in every direction - rotationally invariant.

But I'm struggling to see how 1) and 2) follow from this. As stupid as it sounds, I don't really see where time comes in when these properties are only on the spacelike slices.

Cheers.
 
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binbagsss said:
the metric must take the form...

No; "must" is incorrect. The correct statement is "one can always choose coordinates in which the metric takes the form..." See further comments below.

binbagsss said:
I've read

Reference please? A general note: statements like "I've read" or "I read somewhere" are red flags that you should be giving a specific reference, not a general vague statement. We can't tell whether what you've read is reliable if we can't read it ourselves.

binbagsss said:
Homogenity would be broken if the a(t) was taken outside the metric

What does "taken outside the metric" mean? Does it mean it multiplies the entire RHS, instead of just the spatial part? I'm going to assume it does in the rest of this post.

binbagsss said:
By isotropicity there can be no cross-terms dtdx, dtdy, dtdz.

More precisely, the fact that the spacetime is isotropic means we can always choose coordinates in which there are no cross terms. See further comments below.

binbagsss said:
homogenous means the same throughout - translationally invariant.

Yes.

binbagsss said:
isotropic means the same in every direction - rotationally invariant.

Yes.

binbagsss said:
I'm struggling to see how 1) and 2) follow from this

Is it both 1) and 2) that you don't understand, or just 1)? Your next statement seems to relate to 1), not 2).

binbagsss said:
I don't really see where time comes in when these properties are only on the spacelike slices.

The spacelike slices depend on the coordinates you choose. Statements 1) and 2) are really statements about how you can choose coordinates. I pointed that out above in my response to 2), about what "isotropic" means, but it goes for "homogeneous" too. "Homogeneous" does not mean you can't have ##a(t)## multiply the time part of the metric as well as the spatial part; it means that in a homogeneous spacetime, you can choose coordinates such that the time part of the metric is just ##- dt^2##, a constant, independent of the coordinates. If you choose other coordinates for a homogeneous spacetime, then the time part of the metric might have a function ##a(t)## multiplying it (or a function of any of the coordinates). That doesn't mean the spacetime isn't homogeneous; it means you chose coordinates differently.
 

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