Are singularities part of the manifold?

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SUMMARY

The discussion centers on the relationship between singularities and manifolds in the context of General Relativity (GR) and Special Relativity (SR). Participants clarify that simultaneity is observer-dependent, emphasizing that the expanding Friedmann-Robertson-Walker (FRW) universe cannot be described using a single simultaneity convention. The conversation highlights the implications of Einstein's Equivalence Principle and the relativity of simultaneity, asserting that different families of observers can define congruences in curved spacetimes without contradicting the physics of the universe.

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  • Understanding of General Relativity (GR) and Special Relativity (SR)
  • Familiarity with Friedmann-Robertson-Walker (FRW) cosmology
  • Knowledge of Einstein's Equivalence Principle
  • Concept of simultaneity in curved spacetimes
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Physicists, cosmologists, and students of theoretical physics interested in the foundations of General Relativity and the nature of spacetime. This discussion is particularly beneficial for those exploring the implications of singularities and the relativity of simultaneity in cosmological contexts.

  • #31
It looks to me like everyone is using different definitions of "simultaneity" and "relativity of simultaneity". Maybe we should taboo those terms in this thread, so that everyone has to explicitly define what they mean by them.
 
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  • #32
TrickyDicky said:
This sounds as if it made you mad :mad: that SR is merely local in GR. But if it were global it would be SR not GR don't you think? :rolleyes: :wink:
No, I disagree. If you have a global coordinate chart in GR it doesn't suddenly become SR.
 
  • #33
DaleSpam said:
No, I disagree. If you have a global coordinate chart in GR it doesn't suddenly become SR.

Er...there are no global coordinates (defined as it is standard as those that cover the whole manifold) in curved manifolds, it is one of the most basic facts of differential geometry.
 
  • #34
No, you're thinking of global inertial frames. There's a difference. As an example, Kruskal coordinates for the Schwarzschild space-time cover the entire manifold.
 
  • #35
TrickyDicky said:
Er...there are no global coordinates (defined as it is standard as those that cover the whole manifold) in curved manifolds, it is one of the most basic facts of differential geometry.

You're kidding, right? Some examples of coordinates on curved manifolds that cover the entire manifold:

Kruskal coordinates on maximally extended Schwarzschild spacetime;

FRW coordinates on FRW spacetime (I asked you before about this--are you claiming that FRW coordinates do *not* cover all of FRW spacetime? If so, please show me, explicitly, what part of FRW spacetime FRW coordinates do not cover.)

Any of several standard charts on de Sitter spacetime (any of the ones mentioned in the Wikipedia page would work).

And, of course, a Penrose chart on *any* of the spacetimes I mentioned; Penrose charts are specifically constructed to make sure they cover the entire manifold--and what's more, they do so with a finite range of all coordinates.
 
  • #36
PeterDonis said:
You're kidding, right? Some examples of coordinates on curved manifolds that cover the entire manifold:

Kruskal coordinates on maximally extended Schwarzschild spacetime;

FRW coordinates on FRW spacetime (I asked you before about this--are you claiming that FRW coordinates do *not* cover all of FRW spacetime? If so, please show me, explicitly, what part of FRW spacetime FRW coordinates do not cover.)

Any of several standard charts on de Sitter spacetime (any of the ones mentioned in the Wikipedia page would work).

And, of course, a Penrose chart on *any* of the spacetimes I mentioned; Penrose charts are specifically constructed to make sure they cover the entire manifold--and what's more, they do so with a finite range of all coordinates.

My dear Peter, I'm afraid you are using a rather loose concept of "the whole manifold", it is obvious that all of those charts leave out some point, namely the singularity.
Think about the sphere to make this simpler, according to your use of the term global coordinates you are saying that the sphere can be covered with only one set of global coordinates, after all it only leaves out one point(one of the poles) right? Well I'm afraid not.
 
  • #37
The Schwarzschild singularity is not a part of the space-time manifold. It is an excise, you complement it out. ##S^2## is a completely different situation; the north and south poles are not geometric singularities.
 
  • #38
TrickyDicky said:
My dear Peter, I'm afraid you are using a rather loose concept of "the whole manifold", it is obvious that all of those charts leave out some point, namely the singularity.

The singularity is not part of the manifold in any of the cases I gave. That's why your analogy with a sphere does not hold (not that it matters anyway--see below): a sphere's poles are part of the manifold.

TrickyDicky said:
Think about the sphere to make this simpler, according to your use of the term global coordinates you are saying that the sphere can be covered with only one set of global coordinates

I said no such thing. *You* said "there are no global coordinates in curved manifolds". I responded by saying "there are global coordinates in the following curved manifolds", which is sufficient to refute your claim. I did *not* say "there are global coordinates in *all* curved manifolds", which would, as you say, be false, since a sphere is an obvious counterexample.

You asked earlier in this thread if your use of English was really that bad. Given that you have repeatedly had this same problem, with multiple people, perhaps you should consider the possibility that yes, it is; and that you should take more care to make sure you are actually saying explicitly what you mean, instead of saying something else and expecting us to read your mind and translate what you said into what you actually meant. This would also have the benefit of focusing disagreement much faster; the only thing we appear to disagree about in this particular subthread is that you think singularities are part of the manifold, but it's taken longer than it needed to for us to get to that point.
 
  • #39
PeterDonis said:
The singularity is not part of the manifold in any of the cases I gave.

Take the closed FRW metric, it is Minkowski spacetime plus the singularity point, if it had no singularity it would be flat, ergo the singularity must belong to the manifold in order to be curved, do you get it now?

Hope my english is understandable here.
 
  • #40
WannabeNewton said:
No, you're thinking of global inertial frames. There's a difference. As an example, Kruskal coordinates for the Schwarzschild space-time cover the entire manifold.
No, and I was expecting your usually rigorous use of the math would allow you to see this. Kruskal coordinates don't cover the singularity. Do you also think that the singularity has nothing to do with the manifold?
 
  • #41
TrickyDicky said:
Take the closed FRW metric, it is Minkowski spacetime plus the singularity point

It is no such thing. The closed FRW metric has topology S3 X R; neither the past nor the future singularity are part of the manifold. And there is no relationship that I'm aware of between the closed FRW metric and Minkowski spacetime.

There is an "empty" FRW metric (the Milne model) that is isometric to one "wedge" of Minkowski spacetime (with an unusual coordinate chart), but the "singularity" (which is just the origin of the Minkowski spacetime) is *not* part of the FRW manifold in that case (and it *is* part of the Minkowski spacetime, not an extra point added on to it, so even if it were part of the FRW manifold it wouldn't match your description).

TrickyDicky said:
if it had no singularity it would be flat, ergo the singularity must belong to the manifold in order to be curved, do you get it now?

I get that you are either confused or still not expressing yourself very well.

TrickyDicky said:
Hope my english is understandable here.

I'm not sure, since if I take what you are saying at face value, as above, it is egregiously wrong. So I'm still thinking you meant to say something else; but it's possible that you actually have a seriously mistaken understanding of what you're talking about.
 
  • #42
PeterDonis said:
It is no such thing. The closed FRW metric has topology S3 X R; neither the past nor the future singularity are part of the manifold. And there is no relationship that I'm aware of between the closed FRW metric and Minkowski spacetime.

George Jones said:
...Minkowski space with a point removed is the topological space S^3 x R, the underlying space for the manifold of closed Friedmann-Robertson-Walker universes, ...
Maybe you believe George, it seems you put more effort discrediting what it is said depending on who says it rather than on the content.
 
  • #43
TrickyDicky said:
Maybe you believe George, it seems you put more effort discrediting what it is said depending on who says it that on the content.

No, it depends on saying it correctly, and on understanding what you're saying.

George said "Minkowski space with a point removed" gives the topology S3 X R, the topology of the closed FRW universe. I agree with that.

George did *not* say that the closed FRW universe (or any FRW universe) includes the singularity point. It doesn't.

You said "Minkowski space plus the singularity point", which is *not* what George said; it's wrong in two ways. See above.
 
  • #44
PeterDonis said:
No, it depends on saying it correctly, and on understanding what you're saying.

George said "Minkowski space with a point removed" gives the topology S3 X R, the topology of the closed FRW universe. I agree with that.

George did *not* say that the closed FRW universe (or any FRW universe) includes the singularity point. It doesn't.

You said "Minkowski space plus the singularity point", which is *not* what George said; it's wrong in two ways. See above.
Amusing. The point removed is the singularity point, you know this, don't you?
 
  • #45
TrickyDicky said:
Amusing. The point removed is the singularity point, you know this, don't you?

So what? The point is *removed*--that means it is *not* part of the manifold. Which is what George said, and what I said. And *not* what you said.

How long do you want to keep digging?
 
  • #46
PeterDonis said:
So what? The point is *removed*--that means it is *not* part of the manifold. Which is what George said, and what I said. And *not* what you said.

How long do you want to keep digging?
The funny thing is you understood what i meant all along. Well, it's sad actually.
Let's say that having a point removed is what keeps the manifold from being completely covered with a coordinate chart alone. do you like it more like this?
A singularity is the absence of a point(or points), the absence of a point seems to be a defining part of all the manifolds you mentioned, it is clear that in this sense the singularity(the absence of the point) is part of the manifold, is this clear enough?
 
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  • #47
TrickyDicky said:
Let's say that having a point removed is what keeps the manifold from being completely covered with a coordinate chart alone. do you like it more like this?

[Edited]

Hmm. I see what you're saying [edited again: maybe not, in view of you're subsequent posts, but what follows is still valid], that the S3 part makes it uncoverable by a single chart; but the way you put it makes it sound like the only way to obtain the S3 X R manifold is by removing a point from R4. That's not really true; manifolds are topological spaces in their own right.

Also, none of this changes the fact that the singularity is not part of the manifold. Are you now agreeing with that?
 
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  • #48
  • #49
PeterDonis said:
No. You can cover the entire manifold S3 X R with a single coordinate chart. That's what the standard FRW chart on closed FRW spacetime does.
It is evident it cannot cover a missing point, isn't it? A missing point that is a defining part of the manifold, otherwise it would be Minkowski.
 
  • #50
TrickyDicky said:
It is evident it cannot cover a missing point, isn't it? A missing point that is a defining part of the manifold, otherwise it would be Minkowski.

First, see my edit to that post; the S3 part of the manifold does introduce a complication.

Second, the missing point is not a "defining part" of the manifold; see my edited previous post. S3 X R is a topological space in its own right, independent of the fact that you can "obtain" it by removing a point from R4. (Note that it's R4, not "Minkowski space", because topologically Minkowski space is just R4; it's only when you introduce a metric on it that it becomes Minkowski space, as opposed to all the other geometries that are also topologically R4.)

Third, the fact that the FRW chart does not cover the "missing point" has nothing to do with it not being able to cover the entire manifold; the only reason it can't on closed FRW spacetime is the S3 part of the topology. The FRW charts on flat and open FRW spacetime do cover the entire manifold (which does *not* include the singularity).
 
  • #51
  • #52
PeterDonis said:
Also, none of this changes the fact that the singularity is not part of the manifold. Are you now agreeing with that?

See post above.
But using logic alone, if you say the singularity is not part of the manifold, you are saing that the manifold is singularity-free. See Hawking and Penrose singularity theorems.
 
  • #53
TrickyDicky said:
But using logic alone, if you say the singularity is not part of the manifold, you are saing that the manifold is singularity-free.

Only if you define "singularity-free" in this way. That's not how the term is usually used; see below.

TrickyDicky said:
See Hawking and Penrose singularity theorems.

Which say that geodesics in such a manifold can't be extended to arbitrary values of their affine parameters; physical invariants along them increase without bound as some finite value of the affine parameter is approached. This does not require, and the singularity theorems do not state, that the point at which the affine parameter actually *achieves* the finite value that indicates the singularity (infinite values of physical invariants) is part of the manifold. It only requires that the singularity can be approached arbitrarily closely (where "closely" is defined by the value of the affine parameter along the geodesic of approach) while staying within the manifold.

The term "singularity-free", then, doesn't just mean there are no singularities in the manifold; it means something stronger, that there are no singularities in the manifold *and* that all geodesics can be extended to arbitrary values of their affine parameter with all physical invariants along them remaining finite. I believe Hawking and Ellis explicitly give this definition.
 
  • #54
I mentioned the theorems to indicate that GR manifolds seem to have singularities, otherwise why worry about them?
 
  • #55
TrickyDicky said:
I mentioned the theorems to indicate that GR manifolds seem to have singularities, otherwise why worry about them?

If "singularities" is defined appropriately, I agree. But the appropriate definition does not imply that there are actual points contained in the manifold that are singularities. It only implies what I said in my last post, that a manifold with singularities has geodesics that can't be extended to arbitrary values of their affine parameters.
 
  • #56
PeterDonis said:
If "singularities" is defined appropriately, I agree. But the appropriate definition does not imply that there are actual points contained in the manifold that are singularities.

The fact is there is no definition whatsoever of singularity in GR(only of singular spacetime, which to my surprise according to many is the one that doesn't contain a singularity) unlike in mathematics, so I wonder how it can be appropriately defined at all.
 
  • #57
Hawking and Ellis address your exact misconception in section 8.1
 
  • #58
PeterDonis said:
It looks to me like everyone is using different definitions of "simultaneity" and "relativity of simultaneity". Maybe we should taboo those terms in this thread, so that everyone has to explicitly define what they mean by them.

Totally completely against my better judgement I'm going to step into this thread, just long enough to say that the best definition I've been able to come up with is:

Two events are simultaneous if they have the same time coordinate. This definition makessit clear that that simultaneity is a convention based on the choice of coordinates; and it also allows for the SR definition of simultaneity in which every observer chooses to use the coordinate system in which he is at rest.

Relativity of simultaneity is just the observation that different observers using different coordinate systems will will assign different values of the time coordinate to events, and therefore may disagree about which events have the same time coordinate.
 
  • #59
TrickyDicky said:
The fact is there is no definition whatsoever of singularity in GR(only of singular spacetime, which to my surprise according to many is the one that doesn't contain a singularity) unlike in mathematics, so I wonder how it can be appropriately defined at all.

The sort of singularity that is associated with a black hole can be characterized as the existence of a geodesic such that the curvature increases without bound as you follow the geodesic.
 
  • #60
stevendaryl said:
The sort of singularity that is associated with a black hole can be characterized as the existence of a geodesic such that the curvature increases without bound as you follow the geodesic.

You also have to include that the curvature increases without bound as a finite value of the affine parameter along the geodesic is approached.
 

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