
TL;DR
This paper investigates conditions under which incomplete causal geodesics in spacetimes can be extended, focusing on the role of curvature bounds and singularities, and establishing criteria for global extendibility in general relativity.
Contribution
It provides new criteria for extending incomplete geodesics in globally hyperbolic spacetimes based on curvature bounds and singularity types.
Findings
Existence of local coordinates near incomplete geodesics without tidal or topological singularities.
Conditions for $C^{k-}$ extensions of spacetimes based on curvature and derivative bounds.
Incompleteness terminating on topological singularities implies the spacetime is non-generic.
Abstract
The global extendibility of smooth causal geodesically incomplete spacetimes is investigated. Denote by one of the incomplete non-extendible causal geodesics of a causal geodesically incomplete spacetime . First, it is shown that it is always possible to select a synchronised family of causal geodesics and an open neighbourhood of a final segment of in such that is comprised by members of , and suitable local coordinates can be defined everywhere on provided that does not terminate either on a tidal force tensor singularity or on a topological singularity. It is also shown that if, in addition, the spacetime, , is globally hyperbolic, and the components of the curvature tensor, and its covariant derivatives up to order are bounded on , and also the line…
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