Probing bulk geometry via pole skipping: from static to rotating spacetimes
Cheng Ran, Zhenkang Lu, and Shao-Feng Wu

TL;DR
This paper develops an extended analytical framework for reconstructing complex bulk geometries, including rotating black holes, from pole-skipping boundary data, advancing holographic reconstruction techniques.
Contribution
It generalizes pole-skipping methods to rotating and topological black holes, introduces angular pole-skipping, and links Einstein equations and energy conditions to boundary data constraints.
Findings
Full reconstruction of 3D rotating black holes from boundary data.
Partial reconstruction of Kerr-like spacetimes using radial pole-skipping.
Bulk Einstein equations translate into algebraic constraints on pole-skipping data.
Abstract
We investigate an analytical framework for reconstructing bulk geometries from pole-skipping data. Previously, this method enabled the recursive recovery of near-horizon metric derivatives in static, planar-symmetric black holes. Building on this framework, we systematically extend it to more intricate geometries, specifically static topological black holes and rotating black holes. For three-dimensional rotating black holes, we demonstrate that the metric can be fully reconstructed from boundary pole-skipping data. For four-dimensional rotating spacetimes admitting a separable coordinate system (such as the Kerr family), standard near-horizon pole-skipping successfully reconstructs the purely radial metric functions. To recover the remaining angular metric functions, we introduce a mathematical counterpart termed "angular pole-skipping," defined via a near-axis analysis. Although its…
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.
