I Euclidean geometry and gravity

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In a high-gravity environment, such as near a black hole, the angles of a triangle drawn on a piece of paper may not add up to 180 degrees, particularly if the paper is oriented radially. Observations from a distance complicate interpretations due to light's behavior in curved spacetime, making it difficult to discern non-Euclidean geometry. While the measuring apparatus would not be significantly warped, the effects of gravity can alter the shape of objects in a gravitational field. The geometry of space around a black hole is influenced by the curvature of spacetime, but usable data can still be obtained from gravitational lensing, despite the challenges in interpretation. Ultimately, the geometry of spacetime is a fundamental concept in general relativity, distinct from the geometry of space itself.
  • #151
Jaime Rudas said:
Is that "flat plane" two-dimensional or three-dimensional?

Two dimensional
 
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  • #152
raagamuffin said:
Then I read a reference to 'frame dragging' in rotational black holes. What effect, if any, will that have on the 'paper'?
If the paper is "hovering" statically, i.e., no radial or tangential motion, frame dragging has no effect.
 
  • #153
PAllen said:
In the side discussion of embedding a piece of a plane smoothly, isometrically, in a 3-sphere (following is part of a response to @pervect 's last post:

I thought I would make explicit the construction in that reference (which is presented it very compactly in any number of dimensions). Making it explicit for flat 2-surface section in a 3-sphere, the mechanism is simply to use a properly sized flat torus. As explained in:
https://en.wikipedia.org/wiki/Clifford_torus
a flat torus of just the right size will smoothly fit in a unit 3-sphere, both embedded in R4. But then, the embedding can be just ignored, and you are left with a smooth embedding of a piece of Euclidean plane in a 3-sphere.

The formalization and generalization of this is the general approach to embedding ##E^n## into higher dimesnsional spheres used in the reference I quoted earlier. The general achievement is a local embedding of ##E^n## into an m-sphere, with ##m=2n-1##.

Thank you. Untangling this in terms I can more fully understand will be quite a problem. I'm suspecting the issue is fundamental in that I'm viewing curvature as being defined by a metric. Which isn't necessarily how mathematicains view it.

But I think the discussion has moved outside of what's helpful to the OP's question.
 
  • #154
pervect said:
I'm viewing curvature as being defined by a metric.
More precisely, by the Riemann curvature tensor that's derived from a metric via its Levi-Civita connection. There's no problem with that--that's how the term is being used in this discussion.

But the metric of what? Take the case of a 2-sphere embedded in Euclidean 3-space. The 2-sphere is curved. The 3-space is flat. But one is embedded in the other. How can that be? Taking what you appear to be trying to say at face value, that should be impossible.

The reason it's possible is that the 2-sphere embedded in Euclidean 3-space is a submanifold of that 3-space, and we can define a metric on the submanifold that is curved even though the metric of the 3-space overall is flat. They're simply two different metrics. Note that those metrics give different answers to questions like the distance between two points, even if we restrict the points under consideration to those on the 2-sphere.

What @PAllen has been describing is simply a case where that works in reverse: you have a curved 3-manifold, the 3-sphere, with a submanifold, the Clifford 2-torus, on which a flat metric can be defined. Again, you simply have two different metrics.
 
  • #155
PeterDonis said:
The reason it's possible is that the 2-sphere embedded in Euclidean 3-space is a submanifold of that 3-space, and we can define a metric on the submanifold that is curved even though the metric of the 3-space overall is flat. They're simply two different metrics. Note that those metrics give different answers to questions like the distance between two points, even if we restrict the points under consideration to those on the 2-sphere.
When discussing isometric embeddings, there is a little more to it. The metric of the submanifold is taken to be induced from the manifold metric. This means that, e.g. the distance along a curve on the 2-sphere embedded in E3 is, in fact required to be that same whether you use the manifold metric or the induced metric on the 2-sphere. You get to choose manifold, its metric, and the definition of the submanifold embedded in it as a set of points. You do not then get to choose an arbitrary metric on the submanifold - it is taken to be that induced by the manifold metric.
 
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  • #156
PAllen said:
the distance along a curve on the 2-sphere embedded in E3 is, in fact required to be that same whether you use the manifold metric or the induced metric on the 2-sphere.
Yes. It's important to recognize also that the curve in question is a geodesic of the curved 2-sphere, but it is not a geodesic of the Euclidean 3-space. Considering the implications of that might help @pervect to see what's going on in such cases.
 
  • #157
PAllen said:
a flat torus of just the right size will smoothly fit in a unit 3-sphere
What does "unit" mean in this context?
 
  • #158
Jaime Rudas said:
What does "unit" mean in this context?
Radius of curvature = 1
 
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