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

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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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math.AP 1

years

2026 1

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ACCEPT 1

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Free boundary space-like graphs with prescribed mean curvature

math.AP · 2026-08-01 · accept · novelty 7.0

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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  • Free boundary space-like graphs with prescribed mean curvature math.AP · 2026-08-01 · accept · none · ref 9 · internal anchor

    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.