Meaning of r in Schwarzchild coordinates

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In the discussion about the meaning of "r" in Schwarzschild coordinates, it is clarified that "r" does not represent the distance from the center of a spherical shell to a point on its surface, and the distance between two spherical masses is not simply the difference of their radii due to the curvature of spacetime. The Schwarzschild metric is shown to describe static spacetime geometries, allowing for the identification of hypersurfaces with fixed "r" coordinates, which correspond to 2-spheres. The proper distance between two points at different "r" coordinates is expressed through an integral that indicates it does not equal the coordinate distance. The conversation also emphasizes the need for a proper understanding of "r," particularly outside the Schwarzschild radius, and the complexities involved in defining distances in curved spacetime.
  • #51
I was doing some more reading about the general case, and I suspect that Frobenius' theroem may be involved in the more general solution.

But it's all terribly abstract, I'm not getting much of a "physical" feel.

"Hypersurface orthogonality" is mentioned as a special case of Frobenius' theorem (see pg 434, for instance).
 
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  • #52
pervect said:
I was doing some more reading about the general case, and I suspect that Frobenius' theroem may be involved in the more general solution.

But it's all terribly abstract, I'm not getting much of a "physical" feel.

"Hypersurface orthogonality" is mentioned as a special case of Frobenius' theorem (see pg 434, for instance).
I don't know much about this, but after some reading on the net, it would appear that the theorem only applies to homogenous, linear 1st order PDEs. The EFEs are coupled, non-linear 2nd order PDEs. Can the theorem be applied to GR?
 
  • #54
PWiz said:
it would appear that the theorem only applies to homogenous, linear 1st order PDEs.

Can you give a reference? The discussions I've seen (such as the one in Wald) don't talk about differential equations at all; they talk about manifolds and vector fields or differential forms. (Also, in GR the theorem isn't applied to the EFE; it is applied after you've already solved the EFE, to the manifold with metric that you obtain as the solution.)
 
  • #55
Wikipedia said:
...the theorem addresses the problem of finding a maximal set of independent solutions of a regular system of first-order linear homogeneouspartial differential equations.
I read this. I'll emphasize again - I know nothing about this theorem. I've yet to go through a completely formal treatment in GR and topology.
 
  • #56
PWiz said:
I read this.

Yes; the differential equations referred to are not Einstein's Field Equations, so the fact that the EFE is second-order and nonlinear is irrelevant. The equations referred to are equations describing integral curves of vector fields in a spacetime manifold that is a solution of Einstein's Field Equations. AFAIK those equations are first order and linear. (The Wiki page also describes a geometric interpretation of what is going on, which is much closer to how the theorem is applied in GR.)
 
  • #57
PeterDonis said:
Can you give a reference? The discussions I've seen (such as the one in Wald) don't talk about differential equations at all; they talk about manifolds and vector fields or differential forms. (Also, in GR the theorem isn't applied to the EFE; it is applied after you've already solved the EFE, to the manifold with metric that you obtain as the solution.)

Check "Introduction to Smooth Manifolds" by J.Lee. From page 361: "...explicitly finding integral manifolds boils down to solving a system of PDEs, we can interpret the Frobenius theorem as an existence and uniqueness result for such equations." And then it goes to show this connection.