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We provide strong evidence that, up to $99.999\%$ of extremality, Kerr-Newman black holes (KN BHs) are linear mode stable within Einstein-Maxwell theory.
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K. Glampedakis and N. Andersson, Late time dynamics of rapidly rotating black holes
2001
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E. Berti, V. Cardoso, K. D. Kokkotas, and H. Onozawa, Highly damped quasinormal modes of Kerr black holes
2003
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S. Hod, Slow relaxation of rapidly rotating black holes
2008
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D. Robinson, Four decades of black holes uniqueness theorems
2009
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E. Berti, V. Cardoso, and A. O. Starinets, Quasinormal modes of black holes and black branes
2009
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2012
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2013
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2013
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O. J. Dias and J. E. Santos, Boundary Conditions for Kerr-AdS Perturbations
2013
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2014
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