Domain Structure of Black Hole Space-Times with a Cosmological Constant
Jay Armas, Pawel Caputa, Troels Harmark

TL;DR
This paper extends the concept of domain structures to classify and analyze stationary black hole space-times with a cosmological constant, providing new topological invariants and insights into horizon topologies in various dimensions.
Contribution
It generalizes the domain structure framework to include asymptotically de Sitter and Anti-de Sitter space-times, offering a unified approach for higher-dimensional black hole classification.
Findings
Domain structures for asymptotically Anti-de Sitter space-times resemble flat cases.
Domain structures for asymptotically de Sitter space-times are compact.
Horizon topologies are restricted by the domain structure analysis in certain dimensions.
Abstract
We generalize the domain structure for stationary black hole space-times to include asymptotically de Sitter and Anti-de Sitter space-times. Given a set of commuting Killing vector fields of a space-time the domain structure lives on the submanifold of the orbit space on which at least one of the Killing vector fields has zero norm. In general the domain structure provides topological and geometrical invariants of black hole space-times that in specific cases have proven to be a crucial part of a full characterization leading to uniqueness theorems. In four and five dimensions the domain structure generalizes the rod structure. We examine in detail the domain structure for four, five, six and seven-dimensional black hole space-times including a very general class of spherically symmetric and static black hole space-times as well as the exact solutions for Kerr-(Anti)-de Sitter black…
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.
