Solve General Geodesics in FLRW Metric w/ Conformal Coordinates

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SUMMARY

The discussion focuses on solving general geodesics in the Friedmann-Lemaître-Robertson-Walker (FLRW) metric when transitioning from comoving to conformal coordinates. Participants clarify that the presence of a Killing vector field does not simplify the geodesic equations due to the dependence of metric coefficients on the conformal coordinate, denoted as eta (##\eta##). The conversation highlights two primary methods for computing geodesics: the brute force approach and the geodesic Lagrangian method. Additionally, it is noted that the shape of orbits in FLRW spacetimes is independent of the choice of scale factor, as referenced in the paper by D. Garfinkle.

PREREQUISITES
  • Understanding of the Friedmann-Lemaître-Robertson-Walker (FLRW) metric
  • Familiarity with geodesic equations in general relativity
  • Knowledge of Killing vector fields and their significance
  • Proficiency in differential geometry and tensor calculus
NEXT STEPS
  • Study the geodesic Lagrangian method for solving geodesic equations
  • Review the paper "The shape of the orbit in FLRW spacetimes" by D. Garfinkle
  • Explore the implications of different scale factors on geodesic paths in FLRW metrics
  • Investigate the role of Killing vectors in simplifying geodesic calculations
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Researchers, physicists, and students in cosmology and general relativity, particularly those interested in the dynamics of geodesics in FLRW spacetimes.

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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