Given a globally hyperbolic spacetime M , we show the existence of a smooth spacelike Cauchy hypersurface S and, thus, a global diffeomorphism between M and R × S. * The authors acknowledge Prof. P. Ehrlich's clarifying comments on Geroch's theorem and subsequent references.
To Professor P.E. Ehrlich, wishing him a continued recovery and good health Abstract The folk questions in Lorentzian Geometry which concerns the smoothness of time functions and slicings by Cauchy hypersurfaces, are solved by giving simple proofs of: (a) any globally hyperbolic spacetime (M, g) admits a smooth time function T whose levels are spacelike Cauchy hyperfurfaces and, thus, also a smooth global splitting M = R × S, g = −β(T , x)dT 2 +ḡ T , (b) if a spacetime M admits a (continuous) time function t then it admits a smooth (time) function T with timelike gradient ∇T on all M .
The classical definition of global hyperbolicity for a spacetime (M, g) comprises two conditions: (A) compactness of the diamonds J + (p) ∩ J − (q), and (B) strong causality. Here we show that condition (B) can be replaced just by causality. In fact, we show first that the classical definition of causal simplicity (which impose to be distinguishing, apart from the closedness of J + (p), J − (q)) can be weakened in causal instead of distinguishing. So, the full consistency of the causal ladder (recently proved by the authors in a definitive way) yields directly the result.2000 MSC: Primary 53C50, Secondary 53C80, 83C75.
Recently, folk questions on the smoothability of Cauchy hypersurfaces and time functions of a globally hyperbolic spacetime M , have been solved. Here we give further results, applicable to several problems:(1) Any compact spacelike acausal submanifold H with boundary can be extended to a spacelike Cauchy hypersurface S. If H were only achronal, counterexamples to the smooth extension exist, but a continuous extension (in fact, valid for any compact achronal subset K) is still possible.(2) Given any spacelike Cauchy hypersurface S, a Cauchy temporal function T (i.e., a smooth function with past-directed timelike gradient everywhere, and Cauchy hypersurfaces as levels) with S = T −1 (0) is constructed -thus, the spacetime splits orthogonally as R × S in a canonical way.Even more, accurate versions of this last result are obtained if the Cauchy hypersurface S were non-spacelike (including non-smooth, or achronal but nonacausal). Concretely, we construct a smooth function τ : M → R such that the levels S t = τ −1 (t), t ∈ R satisfy: (i) S = S 0 , (ii) each S t is a (smooth) spacelike Cauchy hypersurface for any other t ∈ R\{0}. If S is also acausal then function τ becomes a time function, i.e., it is strictly increasing on any future-directed causal curve.
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