Solve General Geodesics in FLRW Metric w/ Conformal Coordinates

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Discussion Overview

The discussion revolves around solving general geodesics in the Friedmann-Lemaître-Robertson-Walker (FLRW) metric using conformal coordinates. Participants explore the implications of switching coordinate systems and the challenges associated with calculating geodesics, particularly in scenarios involving motion in multiple dimensions.

Discussion Character

  • Exploratory, Technical explanation, Debate/contested, Mathematical reasoning

Main Points Raised

  • One participant questions whether converting the FLRW metric to conformal coordinates facilitates solving for geodesics, noting the presence of a potential Killing vector.
  • Another participant argues that there is no Killing vector since the metric coefficients depend on the coordinate ##n## (eta), challenging the initial assumption.
  • Some participants suggest that there are straightforward methods for calculating geodesics, including a brute force approach and a geodesic Lagrangian method.
  • One participant proposes that not switching to conformal coordinates might simplify the problem, as the original metric has fewer dependent coefficients.
  • A later reply introduces the idea that the shape of orbits in FLRW spacetimes is independent of the choice of scale factor, which raises questions about the implications of this statement.
  • Another participant expresses skepticism about the claim that the shape of orbits is independent of the scale factor, noting that the duration of following a geodesic may depend on ##a(t)## in certain universes.
  • There is a discussion about the terminology used to describe geodesics with angular momentum, specifically the use of the term "orbit."

Areas of Agreement / Disagreement

Participants express differing views on the utility of conformal coordinates for solving geodesics, with some advocating for their use and others suggesting they complicate the analysis. There is also disagreement regarding the independence of geodesic shapes from the scale factor, indicating unresolved perspectives on this aspect.

Contextual Notes

Some participants note that the analysis of geodesics may depend on specific assumptions about the curvature and the scale factor, which are not fully resolved in the discussion.

Who May Find This Useful

This discussion may be of interest to those studying general relativity, cosmology, or differential geometry, particularly in the context of geodesics and coordinate transformations in FLRW metrics.

Onyx
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TL;DR
Solving for General Geodesics in FLRW Metric
Once having converted the FLRW metric from comoving coordinates ##ds^2=-dt^2+a^2(t)(dr^2+r^2d\phi^2)## to "conformal" coordinates ##ds^2=a^2(n)(-dn^2+dr^2+r^2d\phi^2)##, is there a way to facilitate solving for general geodesics that would otherwise be difficult, such as cases with motion in both ##r## and ##\phi##? I'm curious because there seems to be an ##n## killing vector evident in the new form, but I don't know if that makes it any easier.
 
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Onyx said:
there seems to be an killing vector evident in the new form
No, there isn't, because none of the metric coefficients are independent of ##n## (which is actually the Greek letter eta, ##\eta##, in most treatments in the literature).
 
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PeterDonis said:
No, there isn't, because none of the metric coefficients are independent of ##n## (which is actually the Greek letter eta, ##\eta##, in most treatments in the literature).
It appeared to me that there was, because of ##\frac{\partial K_\eta}{\partial \eta}-\Gamma^{\eta}_{\eta\eta}K_\eta=0##. That's strange.
 
Anyways, I feel like there must be some straightforward way to handle calculating any geodesic in FLRW, but I'm not sure.
 
Onyx said:
It appeared to me that there was, because of ##\frac{\partial K_\eta}{\partial \eta}-\Gamma^{\eta}_{\eta\eta}K_\eta=0##. That's strange.
It's not strange at all. You test for a Killing vector field using Killing's equation, which the equation you wrote down is not. The equation you wrote down is the geodesic equation (well, a somewhat garbled version of it, anyway), and (when properly written) shows that a worldline of constant ##r##, ##\theta##, ##\phi## is a geodesic. Which is not at all strange since that is the worldline of a comoving observer.
 
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Onyx said:
I feel like there must be some straightforward way to handle calculating any geodesic in FLRW
There are two general approaches for computing geodesics. One is the brute force way of writing down all of the components of the general geodesic equation and then eliminating terms which are known to be zero until you have something manageable. The other way, which is considerably faster for metrics like this one where the metric coefficients are only functions of one or two of the coordinates, is the geodesic Lagrangian method, which is described briefly here:

https://en.wikipedia.org/wiki/Solving_the_geodesic_equations#Solution_techniques
 
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Onyx said:
Once having converted the FLRW metric from comoving coordinates ##ds^2=-dt^2+a^2(t)(dr^2+r^2d\phi^2)## to "conformal" coordinates ##ds^2=a^2(n)(-dn^2+dr^2+r^2d\phi^2)##, is there a way to facilitate solving for general geodesics that would otherwise be difficult
One obvious way to make solving for the geodesics easier is to not switch to conformal coordinates. All that does is add one more metric coefficient that depends on a coordinate (##g_{nn}## depends on ##n##, whereas in the original form ##g_{tt}## does not depend on ##t##), and that is going to make more work for you in solving for geodesics no matter what method you use.
 
PeterDonis said:
One obvious way to make solving for the geodesics easier is to not switch to conformal coordinates. All that does is add one more metric coefficient that depends on a coordinate (##g_{nn}## depends on ##n##, whereas in the original form ##g_{tt}## does not depend on ##t##), and that is going to make more work for you in solving for geodesics no matter what method you use.
Perhaps if I consider the form that the metric comes in when switching to ##R=a(t)r##, where there is an ##\frac{a'}{a}## term, setting the scale factor to ##e^t## would help. But it adds a cross-term, so maybe not.
 
Never mind, I actually found a source that provides a way to do it. Apparently, the shape of the orbits is independent of the choice of scale factor, which seems bizarre.
 
  • #10
Onyx said:
I actually found a source that provides a way to do it.
Can you give a reference?

Onyx said:
Apparently, the shape of the orbits is independent of the choice of scale factor
I'm not sure what you mean by "the choice of scale factor".
 
  • #11
PeterDonis said:
Can you give a reference?I'm not sure what you mean by "the choice of scale factor".
"The shape of the orbit in FLRW spacetimes," by D Garfinkle.
 
  • #13
The cited paper notes that the spatial projection of a geodesic in spacetime on to a constant curvature spatial slice (the usual FLRW coordinates' spatial slices) is also a geodesic of that space. Thus the paths depend only on the sign of the curvature and not the details of ##a(t)##.

That doesn't seem to me to be completely true, in that the amount of time for which one can follow a geodesic does depend on ##a(t)## in a closed universe, but that might be overly pedantic.

I note that the paper does not appear to use conformal coordinates in its analysis.
 
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  • #14
Ibix said:
The cited paper notes that the spatial projection of a geodesic in spacetime on to a constant curvature spatial slice (the usual FLRW coordinates' spatial slices) is also a geodesic of that space. Thus the paths depend only on the sign of the curvature and not the details of ##a(t)##.

That doesn't seem to me to be completely true, in that the amount of time for which one can follow a geodesic does depend on ##a(t)## in a closed universe, but that might be overly pedantic.

I note that the paper does not appear to use conformal coordinates in its analysis.
I was thinking only of a ##k=0## case.
 
  • #15
Onyx said:
I was thinking only of a ##k=0## case.
For future reference, is orbit the most frequently used word to describe a geodesic that has angular momentum?
 

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