Asymptotically Flat Spacetime - Formal Definitions

Formal Definitions

A manifold M is asymptotically simple if it admits a conformal compactification such that every null geodesic in M has a future and past endpoints on the boundary of .

Since the latter excludes black holes, one defines a weakly asymptotically simple manifold as a manifold M with an open set UM isometric to a neighbourhood of the boundary of, where is the conformal compactification of some asymptotically simple manifold.

A manifold is asymptotically flat if it is weakly asymptotically simple and asymptotically empty in the sense that its Ricci tensor vanishes in a neighbourhood of the boundary of .

Read more about this topic:  Asymptotically Flat Spacetime

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