On the linear stability of the extreme Kerr black hole under axially symmetric perturbations
Feb 12, 201430 pages
Published in:
- Class.Quant.Grav. 31 (2014) 19, 195009
- Published: Sep 18, 2014
e-Print:
- 1402.2848 [gr-qc]
View in:
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Abstract: (IOP)
We prove that for axially symmetric linear gravitational perturbations of the extreme Kerr black hole, there exists a positive definite and conserved energy. This provides a basic criteria for linear stability in axial symmetry. In the particular case of Minkowski, using this energy we also prove the pointwise boundedness of the perturbation in a remarkably simple way.Note:
- 35 pages. 2 figures. Relevant improvement in the presentation in section 2.2
- 04.20.Ex
- 04.20.Dw
- 04.70.Bw
- stability
- extreme Kerr black hole
References(47)
Figures(2)
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- [9]
- [10]
- [11]
- [12]
- [13]
- [14]
- [15]
- [16]
- [17]
- [18]
- [19]
- [20]
- [21]
- [22]
- [23]
- [24]
- [25]