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A classification theorem for compact Cauchy horizons in vacuum spacetimes

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Abstract

We establish a complete classification theorem for the topology and for the orbital type of the null generators of compact non-degenerate Cauchy horizons of time orientable smooth vacuum \(3+1\)-spacetimes. We show that one and only one of the following must hold: (i) all generators are closed, (ii) only two generators are closed and any other densely fills a two-torus, (iii) every generator densely fills a two-torus, or (iv) every generator densely fills the horizon. We then show that, respectively to (i)–(iv), the horizon’s manifold is either: (i’) a Seifert manifold, (ii’) a lens space, (iii’) a two-torus bundle over a circle, or, (iv’) a three-torus. All the four possibilities are known to arise in examples. In the last case, (iv), (iv’), we show in addition that the spacetime is indeed flat Kasner, thus settling a problem posed by Isenberg and Moncrief for ergodic horizons. The results of this article open the door for a full parameterization of the metrics of all vacuum spacetimes with a compact Cauchy horizon. The method of proof permits direct generalizations to higher dimensions.

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Notes

  1. That is, the quotient of \({\mathbb {R}}^{n}\) by a lattice.

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Acknowledgements

The second author is greatly indebted to Oliver Petersen for letting him know about the important Riemannian metric \(\sigma \) on \({\mathcal {C}}\) invariant under the flow of the vector field V normalizing the surface gravity to a constant.

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  1. Centro de Matemática, Universidad de la República, Montevideo, Uruguay

    Ignacio Bustamante & Martín Reiris

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  1. Ignacio Bustamante
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  2. Martín Reiris
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Correspondence to Martín Reiris.

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Bustamante, I., Reiris, M. A classification theorem for compact Cauchy horizons in vacuum spacetimes. Gen Relativ Gravit 53, 36 (2021). https://doi.org/10.1007/s10714-021-02809-z

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