Spacetime topology is the topological structure of spacetime, a topic studied primarily in general relativity.
This physical theory models gravitation as the curvature of a four dimensional Lorentzian manifold (a spacetime) and the concepts of topology thus become important in analysing local as well as global aspects of spacetime.
The study of spacetime topology is especially important in physical cosmology.
There are two main types of topology for a spacetime M. As with any manifold, a spacetime possesses a natural manifold topology.
[2] Strictly finer than the manifold topology.
It is therefore Hausdorff, separable but not locally compact.
A base for the topology is sets of the form
denote the chronological past and future).
[3] Note that in mathematics, an Alexandrov topology on a partial order is usually taken to be the coarsest topology in which only the upper sets
This topology goes back to Pavel Alexandrov.
Nowadays, the correct mathematical term for the Alexandrov topology on spacetime (which goes back to Alexandr D. Alexandrov) would be the interval topology, but when Kronheimer and Penrose introduced the term this difference in nomenclature was not as clear[citation needed], and in physics the term Alexandrov topology remains in use.
Events connected by light have zero separation.
The plenum of spacetime in the plane is split into four quadrants, each of which has the topology of R2.
The dividing lines are the trajectory of inbound and outbound photons at (0,0).
The planar-cosmology topological segmentation is the future F, the past P, space left L, and space right D. The homeomorphism of F with R2 amounts to polar decomposition of split-complex numbers: F is in bijective correspondence with each of P, L, and D under the mappings z → –z, z → jz, and z → – j z, so each acquires the same topology.
The union U = F ∪ P ∪ L ∪ D then has a topology nearly covering the plane, leaving out only the null cone on (0,0).
Hyperbolic rotation of the plane does not mingle the quadrants, in fact, each one is an invariant set under the unit hyperbola group.