Understanding the phrase "simultaneity convention"

  • I
  • Thread starter Freixas
  • Start date
  • Tags
    Convention
In summary, the question is about the possible range of "simultaneity conventions" in Special Relativity. A "simultaneity convention" is a way of dividing 4-dimensional spacetime into disjoint 3-dimensional subsets, where all events in each subset are defined to happen "at the same time" and are spacelike separated from each other. The possible range of "simultaneity conventions" is any division of spacetime that meets these requirements. The observer's own clock and distance measurements are used in determining "simultaneity conventions."
  • #71
vanhees71 said:
I agree with @PeterDonis, i.e., a useful physical definition of synchronizity should be given by a foliation.
And not just any foliation. For instance a foliation of timelike hypersurfaces may be of interest but I still think it is strange to call it a synchronization convention. In fact if it is not a family of Cauchy surfaces, so that you can study initial value problems, it would be a strange choice of words to call them surfaces of simultaneity.

ps To be fair the paper may be listing that convention just for completeness.
 
  • Like
Likes vanhees71
Physics news on Phys.org
  • #72
martinbn said:
In fact if it is not a family of Cauchy surfaces, so that you can study initial value problems, it would be a strange choice of words to call them surfaces of simultaneity.
While I don't disagree with this, I would point out that it implies that only globally hyperbolic spacetimes can even have "simultaneity conventions" defined in them in the first place. I personally don't think that's much of an issue, since all of the spacetimes we actually use in models of our actual universe or things in it are globally hyperbolic, but it is still a very restrictive condition mathematically.
 
  • Like
Likes martinbn and vanhees71
  • #73
PeterDonis said:
While I don't disagree with this, I would point out that it implies that only globally hyperbolic spacetimes can even have "simultaneity conventions" defined in them in the first place. I personally don't think that's much of an issue, since all of the spacetimes we actually use in models of our actual universe or things in it are globally hyperbolic, but it is still a very restrictive condition mathematically.
I think spacetimes that aren't globally hyperbolic have issues with causality anyway, don't they? Things like CTCs, or removed points? That would make "now" a slippery concept, so perhaps "now is a Cauchy surface" is appropriately restrictive from a physics perspective.
 
  • Like
Likes martinbn and vanhees71
  • #74
PeterDonis said:
While I don't disagree with this, I would point out that it implies that only globally hyperbolic spacetimes can even have "simultaneity conventions" defined in them in the first place. I personally don't think that's much of an issue, since all of the spacetimes we actually use in models of our actual universe or things in it are globally hyperbolic, but it is still a very restrictive condition mathematically.
Yes, but I meant it for the initial value problem. What are other reasons to have a simultaneity convention?
 
  • Like
Likes vanhees71
  • #75
Ibix said:
I think spacetimes that aren't globally hyperbolic have issues with causality anyway, don't they? Things like CTCs, or removed points? That would make "now" a slippery concept, so perhaps "now is a Cauchy surface" is appropriately restrictive from a physics perspective.
If one believes in the strong cosmic censorship conjecture then the non globally hyperbolic ones are the exceptions.
 
  • Like
Likes Ibix and vanhees71
  • #76
Ibix said:
I think spacetimes that aren't globally hyperbolic have issues with causality anyway, don't they? Things like CTCs, or removed points?
Not quite, there are a number of conditions in between globally hyperbolic and spacetimes with those kinds of pathologies. The gory details are in Hawking & Ellis.
 
  • Like
Likes vanhees71 and Ibix
  • #77
PeterDonis said:
The gory details are in Hawking & Ellis.
I think I'll finish Wald first...
 
  • Like
Likes vanhees71
  • #78
martinbn said:
I meant it for the initial value problem. What are other reasons to have a simultaneity convention?
Clock synchronization conventions are useful for all kinds of things. For example, the GPS system has one that doesn't match Einstein clock synchronization (it's impossible to have a global Einstein clock synchronization convention for a rotating congruence of worldlines), but works fine for its intended purpose. Astronomers use a different synchronization convention for labeling events in the solar system, which also works fine for its intended purpose. One might say that part of the intended purpose of at least the latter is solving initial value problems, since the solar system convention is used for things like launching space probes and predicting when they will reach particular mission milestones, but it's certainly not limited to that. But the spacetime in question is globally hyperbolic in any case.
 
  • Like
Likes vanhees71 and martinbn
  • #79
Ibix said:
I think I'll finish Wald first...
Wald Chapter 8 discusses causality conditions, though not to anything like the level of detail that Hawking & Ellis does.
 
  • Like
Likes Ibix and vanhees71
  • #80
PeterDonis said:
Wald Chapter 8 discusses causality conditions, though not to anything like the level of detail that Hawking & Ellis does.
Yeah. Chapter 8 is definitely one I need to revisit...
 
  • Like
Likes vanhees71
  • #81
PeterDonis said:
Clock synchronization conventions are useful for all kinds of things. For example, the GPS system has one that doesn't match Einstein clock synchronization (it's impossible to have a global Einstein clock synchronization convention for a rotating congruence of worldlines), but works fine for its intended purpose. Astronomers use a different synchronization convention for labeling events in the solar system, which also works fine for its intended purpose. One might say that part of the intended purpose of at least the latter is solving initial value problems, since the solar system convention is used for things like launching space probes and predicting when they will reach particular mission milestones, but it's certainly not limited to that. But the spacetime in question is globally hyperbolic in any case.
Well, sometimes pretty local synchronization conventions are sufficient, which should be the case for the GPS and the astronomer's one.
 
  • #82
vanhees71 said:
Well, sometimes pretty local synchronization conventions are sufficient, which should be the case for the GPS and the astronomer's one.
Yes, it all depends on what "pretty local" means. GPS is useful in or near the Earth. The astronomers' convention is useful in the solar system. Those are large regions for us humans, but of course they're extremely small when compared to the universe as a whole.
 
  • Like
Likes vanhees71
  • #83
Sure, but it shows that "FAPP" we only need local concepts like simultaneity conventions, etc.
 
  • #84
PeterDonis said:
A "simultaneity convention" is a way of breaking up the spacetime into disjoint 3-dimensional subsets, such that all of the events in each subset are defined to happen "at the same time". This requires that, for each subset, all of the events in the subset are spacelike separated from each other (meaning that no two events can be connected by a timelike or null curve).
So there is actually a restriction on the type of "constant coordinate time" hypersurfaces allowed to define "a simultaneity convention" i.e. events "at the same time" (i.e. they must be spacelike).

On the other hand any other type of set of 3d hypersurfaces foliating spacetime is good from the point of view of defining a coordinate chart.
 
  • #85
cianfa72 said:
So there is actually a restriction on the type of "constant coordinate time" hypersurfaces allowed to define "a simultaneity convention" i.e. events "at the same time" (i.e. they must be spacelike).
Yes.

cianfa72 said:
On the other hand any other type of set of 3d hypersurfaces foliating spacetime is good from the point of view of defining a coordinate chart.
Strictly speaking, you don't even need a foliation to define a coordinate chart.
 
  • #86
PeterDonis said:
Strictly speaking, you don't even need a foliation to define a coordinate chart.
So in case that coordinate chart has just a local/finite extension in spacetime.
 
  • #87
PeterDonis said:
Strictly speaking, you don't even need a foliation to define a coordinate chart.
Doesn't a coordinate chart imply a foliation, by picking one coordinate and holding it constant? Or does "foliation" imply spacelike planes?
 
  • Like
Likes vanhees71
  • #88
Ibix said:
Doesn't a coordinate chart imply a foliation, by picking one coordinate and holding it constant?
Except in some pathological cases (spacetimes with "holes" in them, etc.--such examples are discussed in Hawking & Ellis), yes, I believe so. But you don't need to define a foliation first in order to define a coordinate chart.

Ibix said:
Or does "foliation" imply spacelike planes?
In some contexts, yes, but I don't believe the general definition does.
 
  • Like
Likes Ibix and vanhees71
  • #89
Ibix said:
does "foliation" imply spacelike planes?
It's worth noting that in globally hyperbolic spacetimes, a foliation by spacelike 3-surfaces always exists--in fact these surfaces are Cauchy surfaces, which means every timelike or null curve intersects the surface exactly once. Many physicists believe that all spacetimes that are actually realizable physically are globally hyperbolic.
 
  • #90
Ibix said:
Doesn't a coordinate chart imply a foliation, by picking one coordinate and holding it constant? Or does "foliation" imply spacelike planes?
A coordinate chart is just a mathematical description of some neighborhood of a differentiable manifold, i.e., a continuous bijective map between an open subset of a Hausdorff point manifold and ##\mathbb{R}^n## with the standard topology (e.g., induced by the Euclidean metric).

It think to do physics you need a bit more, i.e., some notion of a local reference frame and some notion of causal time ordering. This means to do physics you need in fact at least in some local neighborhood a "foliation". That's in order to be able to describe some physical system like "point particles" and "fields" as an initial-value problem of equations of motion describing the "dynamics" of this system.
 
  • #91
Dale said:
I think that nobody wants to allow a coordinate with spacelike integral curves to define a synchronization convention.
Sorry to resume this old thread. I think you mean that nobody wants to allow that a such coordinate (with the feature of having spacelike integral curves) defines a synchronization convention w.r.t. the set of events that share a given value of that coordinate.
 
  • Like
Likes Dale
  • #92
cianfa72 said:
I think you mean that nobody wants to allow that a such coordinate (with the feature of having spacelike integral curves) defines a synchronization convention w.r.t. the set of events sharing a given value of that coordinate.
That is what using a coordinate to define a synchronization convention means.
 
  • Like
Likes Dale and cianfa72
  • #93
Since the thread has been reopened:

Dale said:
I think that nobody wants to allow a coordinate with spacelike integral curves to define a synchronization convention.
Actually that doesn't necessarily indicate a problem. I would say the real problem would be if the surfaces of constant value of the coordinate are not spacelike. (I suppose null surfaces might be acceptable as an edge case, but certainly not timelike.) Spacelike integral curves don't necessarily imply that: for example, inside the horizon of a black hole, the integral curves of the Painleve "time" coordinate ##T## are spacelike, but so are surfaces of constant ##T##, so ##T## can still be, and is, used to define a synchronization convention.
 
  • Like
Likes cianfa72
  • #94
I honestly don’t remember the point I was trying to make with that wording. Sorry.
 
  • #95
PeterDonis said:
Actually that doesn't necessarily indicate a problem. I would say the real problem would be if the surfaces of constant value of the coordinate are not spacelike. (I suppose null surfaces might be acceptable as an edge case, but certainly not timelike.) Spacelike integral curves don't necessarily imply that
Yeah, agreed. That was my concern too.
 
Last edited:
  • #96
PeterDonis said:
I would say the real problem would be if the surfaces of constant value of the coordinate are not spacelike.
Ok, I went back and see what I was saying. I was not speaking of what you are describing here. I was talking about the integral curves, not the surfaces of constant time coordinate, the foliation.

I believe that you agree that the integral curves must be timelike. You additionally want the foliation to be spacelike. The author I cited agrees with the first requirement, but not the second.

So I merely was saying that the first was a consensus requirement, while the second is not. I tend to agree with the spacelike foliation, but I wasn’t expressing my opinion there. I was just expressing the lowest requirement that I think everyone agrees must hold.
 
  • #97
Dale said:
I believe that you agree that the integral curves must be timelike.
@PeterDonis made the example of Painleve coordinate time ##T## inside the black hole horizon: the integral curves are spacelike, however the hypersurfaces of constant Painleve coordinate time ##T=cost## are spacelike as well defining a synchronization convention.
 
  • #98
If you are understanding @PeterDonis position then there may be no consensus requirements at all.

I personally think both requirements should be met.
 
  • #99
Dale said:
I personally think both requirements should be met.
I.e. that both the integral of coordinate curve ##\alpha## (described by other coordinates fixed and varying ##\alpha##) must be timelike and the hypersurfaces of constant ##\alpha## spacelike.
 
Last edited:
  • Like
Likes Dale
  • #100
Dale said:
I believe that you agree that the integral curves must be timelike.
No, I don't. I gave a counterexample: Painleve coordinates inside the horizon of a black hole. The integral curves of ##T## there are spacelike, but so are the surfaces of constant ##T##, so ##T## can be, and is, used to define a simultaneity convention there. That convention is the "natural" one for Painleve observers, i.e., observers free-falling into the hole from rest at infinity, to use; the surfaces of constant ##T## are everywhere orthogonal to the worldlines of Painleve observers (which of course are timelike). But those worldlines are not integral curves of the Killing vector field ##\partial_T##.
 
  • #101
Dale said:
You additionally want the foliation to be spacelike.
I think that would make the most sense, but there are examples of null foliations (for example Eddington-Finkelstein coordinates). I don't think it makes sense for the surfaces of the foliation to have any timelike tangent vectors, and AFAIK there are no examples of proposed foliations that do.
 
  • #102
Dale said:
I personally think both requirements should be met.
I agree that this case (timelike integral curves, spacelike foliation surfaces) will be the one that most clearly matches our intuitive sense of how things should work, and is therefore the most "natural" case.
 
  • Like
Likes cianfa72 and Dale
  • #103
PeterDonis said:
don't think it makes sense for the surfaces of the foliation to have any timelike tangent vectors, and AFAIK there are no examples of proposed foliations that do.
Anderson specifically considers ordinary time zones and the date line as a valid foliation.
 
  • #104
Dale said:
Anderson specifically considers ordinary time zones and the date line as a valid foliation.
Yes, we discussed that before. To recap briefly, time zones and dates don't define a foliation that has timelike tangent vectors on its simultaneity surfaces. They just define different labelings of a foliation whose simultaneity surfaces are all spacelike. For example, if I adjust my clock from Eastern to Central time because I'm traveling, I'm changing coordinate charts, but I'm not changing foliations; both charts use the same foliation, they just label the surfaces differently (a given surface has a Central time label that is 1 hour earlier than its Eastern time label).

Anderson's convention for ##\kappa > 1##, by contrast, has "simultaneity" surfaces that have timelike tangent vectors. I was never able to get a look at the actual paper to see what, if any, argument was made for this, but I don't see how it is the same as time zones and dates. But you are right that it does appear to be a foliation in the published literature that does have simultaneity surfaces with timelike tangent vectors; I had forgotten that example when I made my earlier post.
 
  • #105
PeterDonis said:
To recap briefly, time zones and dates don't define a foliation that has timelike tangent vectors on its simultaneity surfaces. They just define different labelings of a foliation whose simultaneity surfaces are all spacelike.
Reading his paper I don’t think that is what he intended.

PeterDonis said:
For example, if I adjust my clock from Eastern to Central time because I'm traveling, I'm changing coordinate charts, but I'm not changing foliations; both charts use the same foliation, they just label the surfaces differently (a given surface has a Central time label that is 1 hour earlier than its Eastern time label)
I think that is not his intention. I think he intended to allow a foliation such that 9:00 am Eastern is simultaneous with 9:00 am Central. It is an odd approach, but I think that is exactly what he is proposing.

His only stated restriction allows considering 9:00 am Eastern to be simultaneous with 9:00 am Central and the surrounding text supports that message.

To be clear, I don’t like that approach. I have not seen it elsewhere.
 
Back
Top