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In special relativity and general relativity, time and threedimensional space are treated together as a single fourdimensional manifold called spacetime (alternatively, spacetime; see below). A point in spacetime may be referred to as an event. Each event has four coordinates (t, x, y, z).
Just as the x, y, z coordinates of a point depend on the axes one is using, so distances and time intervals, invariant in Newtonian physics, may depend on the reference frame of an observer, in relativistic physics. See length contraction[?] and time dilation[?]. This is the central lesson of special relativity.
The central lesson of general relativity is that spacetime cannot be a fixed background, but is rather a network of evolving relationships.
A spacetime interval between two events is the frameinvariant quantity analogous to distance in Euclidean space. The spacetime interval s along a curve is defined by
where c is the speed of light (some people flip the signs of the equation). A basic assumption of relativity is that coordinate transformations have to leave intervals invariant. Intervals are invariant under Lorentz transformations.
The spacetime intervals on a manifold define a pseudometric[?] called the Lorentz metric[?]. This metric is very similar to distance in Euclidean space. However, note that whereas distances are always positive, intervals may be positive, zero, or negative. Events with a spacetime interval of zero are separated by the propagation of a light signal[?]. Events with a positive spacetime interval are in each other's future or past, and the value of the interval defines the proper time measured by an observer travelling between them. Spacetime together with this pseudometric makes up a pseudoRiemannian manifold[?].
One of the simplest interesting examples of a spacetime is R^{4} with the spacetime interval defined above. This is known as Minkowski space, and is the usual geometric setting for Special Relativity. In contrast, General Relativity says that the underlying manifold will not be flat, if gravity is present, and thus it calls for the use of spacetime rather than Minkowski space.
Strictly speaking one can also consider events in Newtonian physics as a single spacetime. This is GalileanNewtonian relativity[?], and the coordinate systems are related by Galilean transformations. However, since these preserve spatial and temporal distances independently, such a spacetime can be decomposed unarbitrarily, which is not possible in the general case.
A compact manifold can be turned into a spacetime if and only if its Euler characteristic is 0.
Any noncompact 4manifold can be turned into a spacetime.
Many spacetimes have physical interpretations which most physicists would consider bizarre or unsettling. For example, a compact spacetime has closed timelike curves, which violate our usual ideas of causality. For this reason, mathematical physicists usually consider only restricted subsets of all the possible spacetimes. One way to do this is to study "realistic" solutions of the equations of General Relativity. Another way is add some additional "physically reasonable" but still fairly general geometric restrictions, and try to prove interesting things about the resulting spacetimes. The latter approach has lead to some important results, most notably the PenroseHawking singularity theorems[?].
In mathematical physics it is also usual to restrict the manifold to be connected and Hausdorff. A Hausdorff spacetime is always paracompact.
Examples of use of spacetime:
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