Causal structure
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The causal structure of a Lorentzian manifold describes the causal relationships between points in the manifold.
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[edit] Introduction
In modern physics (especially general relativity) spacetime is represented by a Lorentzian manifold. The causal relations between points in the manifold are interpreted as describing which events in spacetime can influence which other events.
Minkowski spacetime is a simple example of a Lorentzian manifold. The causal relationships between points in Minkowski spacetime take a particularly simple form since the space is flat. See Causal structure of Minkowski spacetime for more information.
The causal structure of an arbitrary (possibly curved) Lorentzian manifold is made more complicated by the presence of curvature. Discussions of the causal structure for such manifolds must be phrased in terms of smooth curves joining pairs of points. Conditions on the tangent vectors of the curves then define the causal relationships.
[edit] Tangent vectors
If is a Lorentzian manifold (so g is the metric on the manifold M) then the tangent vectors at each point in the manifold can be classed into three different types. A tangent vector X is
- timelike if
- null if
- spacelike if
(Here we use the metric signature) A tangent vector is called "non-spacelike" if it is null or timelike.
These names come from the simpler case of Minkowski spacetime (see Causal structure of Minkowski spacetime).
[edit] Time-orientability
At each point in M the timelike tangent vectors in the point's tangent space can be divided into two classes. To do this we first define an equivalence relation on pairs of timelike tangent vectors.
If X and Y are two timelike tangent vectors at a point we say that X and Y are equivalent (written ) if .
There are then two equivalence classes which between them contain all timelike tangent vectors at the point. We can (arbitrarily) call one of these equivalence classes "future-directed" and call the other "past-directed". Physically this designation of the two classes of future- and past-directed timelike vectors corresponds to a choice of an arrow of time at the point. The future- and past-directed designations can be extended to null vectors at a point by continuity.
A Lorentzian manifold is time-orientable if a continuous designation of future-directed and past-directed for non-spacelike vectors can be made over the entire manifold.
[edit] Curves
Smooth curves (which possess tangent vectors) in M can be classified depending on their tangent vectors. A smooth curve is
- chronological (or timelike) if the tangent vector is timelike at all points in the curve.
- null if the tangent vector is null at all points in the curve.
- spacelike if the tangent vector is spacelike at all points in the curve.
- causal (or non-spacelike) if the tangent vector is timelike or null at all points in the curve.
Note that these definitions mean that the tangent vector of a chronological curve cannot vanish (i.e. be equal to the zero vector). The tangent vector of a causal curve may vanish.
If the manifold is time-orientable then the non-spacelike curves can further be classified depending on their orientation with respect to time.
A chronological, null or causal curve in the manifold M is
- future-directed if, for every point in the curve, the tangent vector is future-directed.
- past-directed if, for every point in the curve, the tangent vector is past-directed.
These definitions only apply to chronological, null and causal curves because only timelike or null tangent vectors can be assigned an orientation with respect to time.
[edit] Causal relations
There are two types of causal relations between points x and y in the manifold M.
- x chronologically precedes y (often denoted ) if there exists a future-directed chronological (timelike) curve from x to y.
- x causally precedes y (often denoted ) if there exists a future-directed causal (non-spacelike) curve from x to y.
These relations are transitive:
- , implies
- , implies
and satisfy
- implies (this follows trivially from the definition)
- , implies
- , implies
[edit] Causal structure
For a point x in the manifold M we define
- The chronological future of x, denoted , as the set of all points y in M such that x chronologically precedes y:
- The chronological past of x, denoted , as the set of all points y in M such that y chronologically precedes x:
We similarly define
- The causal future (also called the absolute future) of x, denoted , as the set of all points y in M such that x causally precedes y:
- The causal past (also called the absolute past) of x, denoted , as the set of all points y in M such that y causally precedes x:
Points contained in , for example, can be reached from x by a future-directed timelike curve. The point x can be reached, for example, from points contained in by a future-directed non-spacelike curve.
As a simple example, in Minkowski spacetime the set is the interior of the future light cone at x. The set is the full future light cone at x, including the cone itself.
These sets defined for all x in M, are collectively called the causal structure of M.
For S a subset of M we define
For S,T two subsets of M we define
- The chronological future of S relative to T:
- The causal future of S relative to T:
[edit] Properties
- A point x is in if and only if y is in .
Topological properties:
- is open for all points x in M.
- is open for all subsets .
- for all subsets . Here is the closure of a subset S.
[edit] Conformal geometry
Two metrics and are conformally related if for some real function Ω called the conformal factor. (See conformal map).
Looking at the definitions of which tangent vectors are timelike, null and spacelike we see they remain unchanged if we use or As an example suppose X is a timelike tangent vector with respect to the metric. This means that . We then have that so X is a timelike tangent vector with respect to the too.
It follows from this that the causal structure of a Lorentzian manifold is unaffected by a conformal transformation.
[edit] See also
[edit] References
- S.W. Hawking, G.F.R. Ellis, (1973). The Large Scale Structure of Spacetime. Cambridge: Cambridge University Press. ISBN 0-521-20016-4.
- S.W. Hawking, W. Israel, (1979). General Relativity, an Einstein Centenary Survey. Cambridge University Press. ISBN 0-521-22285-0.
- R. Penrose, (1972). Techniques of Differential Topology in Relativity. SIAM. ISBN 0898710057.
[edit] External links
- Turing Machine Causal Networks by Enrique Zeleny, The Wolfram Demonstrations Project.
- Eric W. Weisstein, Causal Network at MathWorld.