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Globally hyperbolic spacetimes can be defined as "causal" instead of "strongly causal"

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arxiv gr-qc/0611138 v1 pith:MXC2JFRK submitted 2006-11-26 gr-qc

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keywords causalcausalityclassicaldefinitiondistinguishinginsteadapartauthors
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abstract

The classical definition of {\em global hyperbolicity} for a spacetime $(M,g)$ comprises two conditions: (A) compactness of the diamonds $J^+(p)\cap J^-(q)$, 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.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Free boundary space-like graphs with prescribed mean curvature

    math.AP 2026-08 accept novelty 7.0 of 10

    The paper proves existence, uniqueness, W^{2,2} regularity and uniform space-likeness for the prescribed Lorentzian mean curvature problem with homogeneous capillary boundary condition on convex domains.

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