Asymptotic structure at timelike infinity: higher orders
Kentaro Tanabe, Tetsuya Shiromizu

TL;DR
This paper investigates the detailed asymptotic structure of four-dimensional spacetimes at timelike infinity under the assumption of asymptotic stationarity, revealing restrictions on the metric form without requiring extra symmetries.
Contribution
It systematically analyzes higher-order asymptotic structures at timelike infinity in stationary spacetimes, highlighting deviations from Kerr black holes without additional symmetry assumptions.
Findings
Asymptotic stationarity imposes strong restrictions on the structure at timelike infinity.
The asymptotic form of the metric deviates from Kerr black holes.
No extra asymptotic symmetries are assumed in the analysis.
Abstract
Bearing the final fate of gravitational collapse in mind, we study the asymptotic structures at timelike infinity in four dimensions. Assuming that spacetimes are asymptotically stationary, we will examine the asymptotic structure of asymptotic stationary spacetimes in a systematic way. Then we see that the asymptotic stationarity strongly restricts the asymptotic structure at timelike infinity. We also observe that the resulted asymptotic form of the metric have the deviation from the Kerr black hole spacetime without assuming of the presence of some additional asymptotic symmetries.
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.
Taxonomy
TopicsAdvanced Mathematical Modeling in Engineering · advanced mathematical theories · Spectral Theory in Mathematical Physics
