CMC existence conjecture for future timelike geodesically complete cosmological spacetimes

Let (M,g)(M,g) be a spacetime with compact Cauchy surfaces. A CMC Cauchy surface is a spacelike Cauchy surface with constant mean curvature. The strong energy condition is the condition

Ric(X,X)0\emph{Ric}(X,X) \geq 0

for all timelike vectors XX.

CMC existence conjecture. If (M,g)(M,g) is future timelike geodesically complete and satisfies the strong energy condition, then (M,g)(M,g) contains a CMC Cauchy surface.

A theorem establishes this conclusion under the stronger assumption of everywhere nonpositive timelike sectional curvature. The conjecture asks whether the strong energy condition alone suffices; its resolution is not specified in the supplied text.

Sources & referencesView supporting material

Primary source

Gregory J. Galloway and Eric Ling, “A CMC existence result for expanding cosmological spacetimes”, arXiv:2410.16619 (2026).

Additional references

2 papers in this index state this conjecture (2019–2024). The statement above is taken from the most recent of them; the others are arXiv:1902.08803.

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