Algorithmic characterization results for the Kerr-NUT-(A)dS space-time. I. A space-time approach
DOI10.1063/1.4980067zbMath1365.83005arXiv1701.02959OpenAlexW2577256880MaRDI QIDQ2981032
Publication date: 8 May 2017
Published in: Journal of Mathematical Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1701.02959
Black holes (83C57) Applications of differential geometry to physics (53Z05) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Gravitational energy and conservation laws; groups of motions (83C40) Equations of motion in general relativity and gravitational theory (83C10)
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Cites Work
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- Rigidity of stationary black holes with small angular momentum on the horizon
- On the construction of a geometric invariant measuring the deviation from Kerr data
- Characterizations of the Kerr metric
- On the uniqueness of smooth, stationary black holes in vacuum
- Radiation states and the problem of energy in general relativity
- A set of invariant quality factors measuring the deviation from the Kerr metric
- A spacetime characterization of the Kerr-NUT-(A)de Sitter and related metrics
- Spacetime Ehlers group: transformation law for the Weyl tensor
- Characterization of (asymptotically) Kerr–de Sitter-like spacetimes at null infinity
- Spacetime characterizations of Λ-vacuum metrics with a null Killing 2-form
- Algorithmic characterization results for the Kerr-NUT-(A)dS space-time. II. KIDs for the Kerr-(A)(de Sitter) family
- Killing spinors as a characterisation of rotating black hole spacetimes
- The ‘non-Kerrness’ of domains of outer communication of black holes and exteriors of stars
- Closed conformal Killing–Yano tensor and the uniqueness of generalized Kerr–NUT–de Sitter spacetime
- An intrinsic characterization of the Kerr metric
- Covariant determination of the Weyl tensor geometry
- Uniqueness properties of the Kerr metric
- A spacetime characterization of the Kerr metric
- Symmetric Tensors and Symmetric Tensor Rank
- Classification of Kerr–de Sitter-like spacetimes with conformally flat $\mathscr{I}$
- The classification of spaces defining gravitational fields
- Uniqueness of smooth stationary black holes in vacuum: Small perturbations of the Kerr spaces
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