New Reply

The topology of spacetimes

 
Share Thread Thread Tools
Jan3-13, 05:35 AM   #52
 

The topology of spacetimes


Quote by WannabeNewton View Post
That is the subset of M generated by null geodesics emanating from p but you are talking about light cones as they relate to causal structure.
That is the point, it is hard to find (at least for me) mathematical justification for deriving a causal structure for the whole manifold only from the local action of the pseudoriemannian metric at the tangent space, when the distance function that prevails in smooth manifolds is not even the same as the one that integrates from the pseudoriemannian metric tensor.
 
Jan3-13, 05:49 AM   #53
 
Mentor
Quote by zonde View Post
If we say that spacetime is Hausdorff then we can't include complete lightcones in the neighborhood of an event.
As has been indicated, some care is needed with respect to the meaning of "lightcone". Depending on the context and reference, "lighcone at [itex]p[/itex]" can either mean a subset of [itex]T_p \left(M\right)[/itex], or it can mean a subset of [itex]M[/itex]. I think that you mean the latter. In this case, [itex]M[/itex] is a neighbourhood of [itex]p[/itex] that contains its light cone.
 
Jan3-13, 06:41 AM   #54
 
Mentor
Quote by zonde View Post
Fine there is someone else who thinks like you.
Now can you provide arguments? In that link there is only definition (belief) and no arguments.

Why do you believe that all spacetimes are Hausdorff?
Quote by atyy View Post
All the usual spacetimes are of course Hausdorff. But just for interest, Hawking and Ellis mention one example of a non-Hausdorff spacetime, and mention a paper by Hajicek.
We want to model physics. For most situations, spacetime Hausdorffness seems to be a reasonable, physical separation axiom. Two distinct physical events always admit distinct neighbouhoods.

Having said this, we have strayed far off-topic with respect to the original post. Physics Forums rules advises that, instead of posts that are off-topic, new threads should be started.
 
Jan3-13, 08:11 AM   #55
 
Blog Entries: 9
Recognitions:
Homework Helper Homework Help
Science Advisor Science Advisor
IMHO, off-topic or not, this is by far the best thread in the Relativity section for quite some time. :)
 
Jan3-13, 08:15 AM   #56
 
Blog Entries: 8
Recognitions:
Gold Membership Gold Member
Science Advisor Science Advisor
Retired Staff Staff Emeritus
I have moved the off-topic posts to a new thread so we can keep discussing this.
 
Jan3-13, 10:00 AM   #57
 
Mentor
Quote by DaleSpam View Post
OK, I guess they must just use the length of the shortest path, regardless of whether or not there are multiple geodesics.
Almost. Consider [itex]\mathbb{R}^2[/itex] with its standard positive-definite norm. Now obtain a new Riemannian manifold M by removing the origin. In this new manifold M, what is the distance between the points (-1 , 0) and (1 , 0)? There is no geodesic in M that joins these points. There isn't even a shortest path in M that joins these points points, i.e., if someone gives me a path in M between (-1 , 0) and (1 , 0), I can always find a shorter path in M.

This leads to a slightly subtle definition of distance in a Riemannian manifold. The distance between points p and q is the greatest bound on the lengths of all "nice" paths between p and q.

In my example, 2 is greatest lower bound of the lengths of paths between, even though there is no path of length 2, and 2 is the distance between (-1 , 0) and (1 , 0).
 
Jan3-13, 10:23 AM   #58
 
Mentor
Quote by WannabeNewton View Post
Indeed even though the two topological spaces mentioned are homeomorphic, they need not have same distance functions. Metrizable implies there exists some metric for the set but it doesn't state there is a single, unique metric. By the way, I think there is some confusion arising here in the terminology.
OK, from my understanding a metric space must have a unique distance between any two points in the space. A metrizable space seems to be one that can be given a metric, not necessarily one that has a metric. So a differentiable manifold is metrizable, but by itself that doesn't make it a metric space. You know that you can equip it with a metric, and once you do so then it is a metric space, not before. Does that agree with your understanding?

Quote by George Jones View Post
Almost. Consider [itex]\mathbb{R}^2[/itex] with its standard positive-definite norm. Now obtain a new Riemannian manifold M by removing the origin. In this new manifold M, what is the distance between the points (-1 , 0) and (1 , 0)? There is no geodesic in M that joins these points. There isn't even a shortest path in M that joins these points points, i.e., if someone gives me a path in M between (-1 , 0) and (1 , 0), I can always find a shorter path in M.

This leads to a slightly subtle definition of distance in a Riemannian manifold. The distance between points p and q is the greatest bound on the lengths of all "nice" paths between p and q.

In my example, 2 is greatest lower bound of the lengths of paths between, even though there is no path of length 2, and 2 is the distance between (-1 , 0) and (1 , 0).
Thanks, that helps my understanding. So what happens for spacelike paths? Also, you should be able to connect any pair of events with a null path, how are those avoided?
 
Jan3-13, 10:32 AM   #59
 
Blog Entries: 8
Recognitions:
Gold Membership Gold Member
Science Advisor Science Advisor
Retired Staff Staff Emeritus
Quote by George Jones View Post
Almost. Consider [itex]\mathbb{R}^2[/itex] with its standard positive-definite norm. Now obtain a new Riemannian manifold M by removing the origin. In this new manifold M, what is the distance between the points (-1 , 0) and (1 , 0)? There is no geodesic in M that joins these points. There isn't even a shortest path in M that joins these points points, i.e., if someone gives me a path in M between (-1 , 0) and (1 , 0), I can always find a shorter path in M.

This leads to a slightly subtle definition of distance in a Riemannian manifold. The distance between points p and q is the greatest bound on the lengths of all "nice" paths between p and q.

In my example, 2 is greatest lower bound of the lengths of paths between, even though there is no path of length 2, and 2 is the distance between (-1 , 0) and (1 , 0).
I wonder what exactly the problem is in this example. Intuitively, the problem is of course the hole at the origin. But is there a condition that we can place on our manifold such that this situation doesn't arise? I guess I'm asking for a condition where there always exists a shortest path.
 
Jan3-13, 10:33 AM   #60
 
Recognitions:
Gold Membership Gold Member
Science Advisor Science Advisor
Quote by DaleSpam View Post
Does that agree with your understanding?
Yessir.
 
Jan3-13, 10:51 AM   #61
 
Blog Entries: 8
Recognitions:
Gold Membership Gold Member
Science Advisor Science Advisor
Retired Staff Staff Emeritus
Quote by micromass View Post
I wonder what exactly the problem is in this example. Intuitively, the problem is of course the hole at the origin. But is there a condition that we can place on our manifold such that this situation doesn't arise? I guess I'm asking for a condition where there always exists a shortest path.
I guess the Hopf-Rinow theorem partially answers this. Any connected and complete Riemannian manifold has length-minimizing geodesics: http://en.wikipedia.org/wiki/Hopf%E2%80%93Rinow_theorem
But this is not an iff-condition. For example, (0,1) also has length-minimizing geodesics but is not complete.
 
Jan3-13, 11:01 AM   #62
 
Mentor
Quote by micromass View Post
I wonder what exactly the problem is in this example. Intuitively, the problem is of course the hole at the origin. But is there a condition that we can place on our manifold such that this situation doesn't arise? I guess I'm asking for a condition where there always exists a shortest path.
Completeness, i.e., convergence of Cauchy sequences and/or geodesic completenss.

"Riemannian Manifolds: An Introduction to Curvature" by Lee has interesting stuff (again!) about this on pages 108-111. For example:
A connected Riemannian manifold is geodesically complete if and only if it is complete as as a metric space.

M is complete if and only if any two points of M can be joined by a minimizing geodesic segment.
[edit]Didn't see the previous post.[/edit]
 
Jan3-13, 11:16 AM   #63
 
Mentor
Quote by micromass View Post
For example, (0,1) also has length-minimizing geodesics but is not complete.
Aha! I coudn't see anything wrong with this, so I looked up the errata for Lee's Book. The second Lee statement that I quoted is wrong! Not iff. See reference to page 111 in

http://www.math.washington.edu/~lee/...ian/errata.pdf
 
Jan3-13, 11:33 AM   #64
 
Mentor
Quote by DaleSpam View Post
Thanks, that helps my understanding. So what happens for spacelike paths? Also, you should be able to connect any pair of events with a null path, how are those avoided?
I make a distinction between "Riemannian" and "semi-Riemannian". What I wrote only applies to Riemannian manifolds.
 
Jan3-13, 12:13 PM   #65
 
Quote by WannabeNewton View Post
Any topological manifold is metrizable. As the requirement is a topological manifold, this is done before a riemannian or pseudo riemannian metric is even equipped to the manifold.
Let me just clear up these definitions, from wikipedia/metric:

In mathematics, a metric or distance function is a function which defines a distance between elements of a set. A set with a metric is called a metric space. A metric induces a topology on a set but not all topologies can be generated by a metric. A topological space whose topology can be described by a metric is called metrizable.
In differential geometry, the word "metric" may refer to a bilinear form that may be defined from the tangent vectors of a differentiable manifold onto a scalar, allowing distances along curves to be determined through integration. It is more properly termed a metric tensor.
So, a metric and our metric tensor are not the same thing, as already said before in this thread, a metric or distance is a map [itex] M\times M\longrightarrow \mathbb{R} [/itex] while the metric tensor is a map [itex] T_pM\times T_pM\longrightarrow \mathbb{R} [/itex].

A topological manifold is it metrizable, i.e. can its topology be described by a distance (may we use an atlas and [itex]\mathbb{R}^n[/itex] euclidean distance)? If yes, which distance? If not, what is then the topology of space time? Secondly, how can we use the fact that spacetime is not only a topological manifold, but a (pseudo-)Riemannian one, to help us on this task?
 
Jan3-13, 01:44 PM   #66
 
Let me just clear up these definitions, from wikipedia/metric:



So, a metric and our metric tensor are not the same thing, as already said before in this thread, a metric or distance is a map [itex] M\times M\longrightarrow \mathbb{R} [/itex] while the metric tensor is a map [itex] T_pM\times T_pM\longrightarrow \mathbb{R} [/itex].

A topological manifold is it metrizable, i.e. can its topology be described by a distance (may we use an atlas and [itex]\mathbb{R}^n[/itex] euclidean distance)?
Well, its topology must look locally Euclidean if it is to be called a manifold, the global geometry(topology) doesn't have to.
But the important thing here is to separate the distance function from the topology, it is true that a metric distance function can induce a topology on a metrizable space, but this is not the case with manifolds, wich carry their own topology.
If yes, which distance? If not, what is then the topology of space time?
See above.

Secondly, how can we use the fact that spacetime is not only a topological manifold, but a (pseudo-)Riemannian one, to help us on this task?
No need, it so happens that differentiable manifolds always admit a Riemannian metric.
 
Jan3-13, 02:01 PM   #67
 
Quote by George Jones View Post
I make a distinction between "Riemannian" and "semi-Riemannian". What I wrote only applies to Riemannian manifolds.

This is confusing. I thought we agreed the distance function on the manifold doesn't distinguish Riemannian metric tensor from semi-riemannian metric tensor since they act locally on the tangent space rather than on the global manifold, and differentiable manifolds topological requirements only allow them to be metric spaces (can't be semimetric nor pseudometric spaces by definition, first of all because they are required to be Haussdorf). So I think Dalespam's question are relevant here.

This is related to what I commented in posts #41, #44 and #52. So far have been ignored, care to give it a try and address them? Thanks George.
 
Jan3-13, 07:09 PM   #68
 
Recognitions:
Science Advisor Science Advisor
Is a Hausdorff space necessarily a metric space? Wikipedia just says thart pseudometric spaces are typically not Hausdorff, but that seems to allow that Hausdorff spaces can be neither metric nor pseudometric. If that is possible, then wouldn't it be possible that Hausdorff manifolds with pseudo-Riemannian metric tensors need not be metric spaces?
 
New Reply
Thread Tools


Similar Threads for: The topology of spacetimes
Thread Forum Replies
The usual topology is the smallest topology containing the upper and lower topology Topology and Analysis 2
The usual topology is the smallest topology containing the upper and lower topology Calculus & Beyond Homework 0
when are two spacetimes the same Special & General Relativity 1
A democracy of spacetimes? Beyond the Standard Model 10
Stringy spacetimes Beyond the Standard Model 0