Asymptotia of Kerr-de Sitter Black Holes

Fuente: arXiv
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Main Authors: Blitz, Samuel, Kopiński, Jarosław
Format: Preprint
Published: 2025
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author Blitz, Samuel
Kopiński, Jarosław
author_facet Blitz, Samuel
Kopiński, Jarosław
contents Exterior geometries of physical black holes are believed to asymptotically approach the Kerr--de Sitter spacetime at late times. A characteristic feature of that vacuum Einstein solution is the presence of a hidden symmetry generated by a closed conformal Killing--Yano tensor. Using this symmetry and modern conformal geometry technology, we find necessary conditions for generic solutions to asymptotically approach the Kerr--de Sitter metric. Further, we constrain the admissible form of the geometric free data on the conformal infinity giving rise to this family of spacetimes and constrain it in terms of the stress-energy tensor.
format Preprint
id arxiv_https___arxiv_org_abs_2506_18169
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Asymptotia of Kerr-de Sitter Black Holes
Blitz, Samuel
Kopiński, Jarosław
General Relativity and Quantum Cosmology
Differential Geometry
Exterior geometries of physical black holes are believed to asymptotically approach the Kerr--de Sitter spacetime at late times. A characteristic feature of that vacuum Einstein solution is the presence of a hidden symmetry generated by a closed conformal Killing--Yano tensor. Using this symmetry and modern conformal geometry technology, we find necessary conditions for generic solutions to asymptotically approach the Kerr--de Sitter metric. Further, we constrain the admissible form of the geometric free data on the conformal infinity giving rise to this family of spacetimes and constrain it in terms of the stress-energy tensor.
title Asymptotia of Kerr-de Sitter Black Holes
topic General Relativity and Quantum Cosmology
Differential Geometry
url https://arxiv.org/abs/2506.18169