Levi-Civita connection and pseudoRiemannian metric

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SUMMARY

The discussion centers on the properties of the Levi-Civita connection in relation to pseudoRiemannian metrics. It is established that the Levi-Civita connection preserves the metric tensor at each point's tangent space, which is crucial for defining invariant intervals in the manifold. The participants clarify that while every manifold can be treated as a metric space, the nuances of distance functions, particularly in the context of null curves and geodesics, require careful consideration. The conversation emphasizes the distinction between metric spaces and metric tensors, asserting that the metric is defined independently of any connection.

PREREQUISITES
  • Understanding of Levi-Civita connection and its properties
  • Familiarity with pseudoRiemannian metrics and their implications
  • Knowledge of geodesics and null curves in differential geometry
  • Basic concepts of metric spaces and topology
NEXT STEPS
  • Explore the properties of the Levi-Civita connection in General Relativity
  • Study the implications of pseudoRiemannian metrics on geodesics
  • Investigate the definition and properties of distance functions in pseudoRiemannian manifolds
  • Learn about the differences between Riemannian and pseudoRiemannian geometries
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Mathematicians, physicists, and students of differential geometry interested in the intricacies of connections, metrics, and their applications in General Relativity.

  • #91
Just out of curiosity, what is the point of this thread?
 
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  • #92
TrickyDicky said:
In the text it is literally stated "we need to calculate the null geodesic from G1 to us".

Which, taken in context, means "find an expression for ##\int ds = 0## along the null geodesic, and then split it up into pieces that have different physical interpretations". What the text does *not* say is anything along the lines of "these separate pieces, even though they have obvious physical interpretations as integrals along timelike or spacelike geodesics, are actually integrals of some function other than ##ds = 0## along the null geodesic the light follows".

TrickyDicky said:
Calculations based on the integration of the null geodesic equations

I'm not sure what you mean by "integration of the null geodesic equations". Finding an expression for ##\int ds = 0## is not the same as integrating the geodesic equation; the ##\int ds = 0## expression can be written down purely from the FRW line element. The geodesic equation itself doesn't appear anywhere in the integrand.

TrickyDicky said:
Hairsplitting whether thy are about "how far" or "how long" or whether each integral by itself is the integral of a null geodesic is a purely terminologic discussion that is of not much utility in practice.

If you mean you don't need to go into all these details in order to get a numerical answer, of course you're right. But the same can be said of hairsplitting about whether what we are doing can be interpreted as calculating a "distance" along the null geodesic that's different from the physical ##ds = 0## distance (i.e., whether we can interpret what we're doing as calculating ##D_T## instead of ##D_M##), as opposed to splitting up the ##\int ds = 0## expression into pieces with obvious physical interpretations as integrals along timelike or spacelike geodesics. None of these interpretations matter if all you're concerned with is getting a numerical answer for ##D_p##. They only matter if you have particular preferences for how to justify interpreting ##D_p## as a "distance".
 
  • #93
PeterDonis said:
Which, taken in context, means "find an expression for ##\int ds = 0## along the null geodesic, and then split it up into pieces that have different physical interpretations". What the text does *not* say is anything along the lines of "these separate pieces, even though they have obvious physical interpretations as integrals along timelike or spacelike geodesics, are actually integrals of some function other than ##ds = 0## along the null geodesic the light follows".
I am saying(like you I think) that they are integrals of ##ds = 0## along the null geodesic the light follows.


I'm not sure what you mean by "integration of the null geodesic equations". Finding an expression for ##\int ds = 0## is not the same as integrating the geodesic equation; the ##\int ds = 0## expression can be written down purely from the FRW line element. The geodesic equation itself doesn't appear anywhere in the integrand.
Right, the sentence is read:integration of the "null geodesic" equations (ds=0), not integration of the null "geodesic equations".


If you mean you don't need to go into all these details in order to get a numerical answer, of course you're right. But the same can be said of hairsplitting about whether what we are doing can be interpreted as calculating a "distance" along the null geodesic that's different from the physical ##ds = 0## distance (i.e., whether we can interpret what we're doing as calculating ##D_T## instead of ##D_M##), as opposed to splitting up the ##\int ds = 0## expression into pieces with obvious physical interpretations as integrals along timelike or spacelike geodesics. None of these interpretations matter if all you're concerned with is getting a numerical answer for ##D_p##. They only matter if you have particular preferences for how to justify interpreting ##D_p## as a "distance".
Fair enough.
Since there is some curiosity about the point of this thread and just in case you are interested in what goes on beyond the purely computational side of it, the chapter "On the structure of space-time" page 178(in google books preview) in the book "Space, time and geometry" is what inspired my OP.
 
  • #94
Do you mean the book by P. Suppes? I must say that I have absolutely no idea how that page of the book led you to this question!
 
  • #95
martinbn said:
Do you mean the book by P. Suppes? I must say that I have absolutely no idea how that page of the book led you to this question!

Yes, that book. But that is just the first page in the essay, he mentions metric spaces and how this definition applies to relativity and classical space-times in pge 180.
 

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