The first fully non-perturbative quasinormal mode spectrum (polar, axial, scalar) for rapidly rotating Einstein-Gauss-Bonnet-dilaton black holes is computed and shown to deviate from Kerr, with mode ordering depending on coupling and spin.
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Quasinormal mode spectrum of rotating black holes in Einstein-Gauss-Bonnet-dilaton theory
The first fully non-perturbative quasinormal mode spectrum (polar, axial, scalar) for rapidly rotating Einstein-Gauss-Bonnet-dilaton black holes is computed and shown to deviate from Kerr, with mode ordering depending on coupling and spin.