Topology of Event Horizons and Topological Censorship
Ted Jacobson, Shankar Venkataramani

TL;DR
This paper proves that, under certain conditions, the event horizon of a four-dimensional asymptotically flat black hole must have a spherical topology, extending topological censorship without assuming stationarity.
Contribution
The authors establish a topological censorship theorem for black hole horizons without requiring stationarity, showing that the horizon topology must be a 2-sphere under broad conditions.
Findings
Horizon cross sections are topologically 2-spheres.
Homology groups of certain submanifolds are finite.
Horizon topology is constrained to be spherical or nonorientable with a projective plane boundary.
Abstract
We prove that, under certain conditions, the topology of the event horizon of a four dimensional asymptotically flat black hole spacetime must be a 2-sphere. No stationarity assumption is made. However, in order for the theorem to apply, the horizon topology must be unchanging for long enough to admit a certain kind of cross section. We expect this condition is generically satisfied if the topology is unchanging for much longer than the light-crossing time of the black hole. More precisely, let be a four dimensional asymptotically flat spacetime satisfying the averaged null energy condition, and suppose that the domain of outer communication to the future of a cut of is globally hyperbolic. Suppose further that a Cauchy surface for is a topological 3-manifold with compact boundary in , and is a compact submanifold of with…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
