Exploring the General Form of FLRW Metric

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Discussion Overview

The discussion revolves around the general form of the Friedmann-Lemaître-Robertson-Walker (FLRW) metric in cosmology, specifically how to incorporate the curvature parameter \( K \) into the metric. Participants explore the implications of different curvature values and seek clarification on the formulation of the metric.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • One participant presents the generic form of the FLRW metric and the three-dimensional spatial metrics for different curvature cases (K=0, K=1, K=-1).
  • Another participant suggests that including \( K \) in the formula as \( dl^2=a^2(\frac{dr^2}{1-Kr^2})+r^2d\Omega^2 \) could yield the desired cases.
  • A participant expresses uncertainty about whether the suggestion is presented ironically or if it is indeed the correct approach.
  • Another participant confirms that the proposed method is correct and that plugging in values for \( K \) leads to the specific line elements.

Areas of Agreement / Disagreement

There is some agreement on the method of incorporating \( K \) into the metric, but uncertainty remains regarding the tone and intent of the suggestions made by participants. The discussion does not reach a consensus on the interpretation of the responses.

Contextual Notes

Participants have not fully resolved the implications of the curvature parameter \( K \) in the context of the FLRW metric, and there are assumptions about the understanding of curvature in cosmological models that are not explicitly stated.

Fleet
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Hi all,

I have found the "generic" form of the FLRW metric:
[tex]ds^2=(cdt)^2-dl^2[/tex]

And I have found the three-dimension spatial metric for euclidian space (K=0, spherical space K=1 and hyperboloid space (K=-1):

[tex]dl^2=a^2(dr^2+r^2d\Omega^2)[/tex]

[tex]dl^2=a^2(\frac{dr^2}{1-r^2})+r^2d\Omega^2)[/tex]

[tex]dl^2=a^2(\frac{dr^2}{1+r^2})+r^2d\Omega^2)[/tex]

BUT how do I find the "general" form of the FLRW metric, how can I include the curvature parameter K?

Please help, I really need it!

Best regards.
 
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What happens if you just stick a K into the formula, with the understanding that it can take on just those 3 values: -1,0,and 1? Don't you get the three cases you want?

[tex]dl^2=a^2(\frac{dr^2}{1-Kr^2})+r^2d\Omega^2)[/tex]

Fleet said:
Hi all,

I have found the "generic" form of the FLRW metric:
[tex]ds^2=(cdt)^2-dl^2[/tex]

And I have found the three-dimension spatial metric for euclidian space (K=0, spherical space K=1 and hyperboloid space (K=-1):

[tex]dl^2=a^2(dr^2+r^2d\Omega^2)[/tex]

[tex]dl^2=a^2(\frac{dr^2}{1-r^2})+r^2d\Omega^2)[/tex]

[tex]dl^2=a^2(\frac{dr^2}{1+r^2})+r^2d\Omega^2)[/tex]

BUT how do I find the "general" form of the FLRW metric, how can I include the curvature parameter K?
...
 
Thank you very much for you answer, I really appreciate it!

Yes, you are right I get the cases I want. But are you questioning to be ironical or are you sure it the correct way? :)

Love this forum, I'm going to contribute

Best regards
 
Fleet said:
Yes, you are right I get the cases I want. But are you questioning to be ironical or are you sure it the correct way? :)

It is the correct way. The general form for the line element is the one that marcus gives. Plugging in values for k gives you the three specific line elements.
 

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