Towards uniqueness of degenerate axially symmetric Killing horizon
arXiv:1206.5136 · doi:10.1007/s10714-013-1506-0
Abstract
We examine the linearized equations around extremal Kerr horizon and give some arguments towards stability of the horizon with respect to generic (non-symmetric) linear perturbation of near horizon geometry.
arXiv comment17 pages
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Cited by in corpus (10)
- Classification of near-horizon geometries of extremal black holes
- The Near Horizon Geometry Equation on Compact 2-Manifolds Including the General Solution for g > 0
- The Petrov type D isolated null surfaces
- Spacetimes foliated by non-expanding and Killing horizons: higher dimension
- Towards a classification of vacuum near-horizons geometries
- Near Horizon Geometries and Black Hole Holograph
- Axisymmetric, extremal horizons in the presence of a cosmological constant
- Rigidity of the extremal Kerr-Newman horizon
- When Isolated Horizons met Near Horizon Geometries
- Extremal Black Holes from Homotopy Algebras