Scalar probe spectra on new rotating black holes and solitons in 5D Einstein-Gauss-Bonnet gravity give gapped mass towers, real soliton frequencies, and rotation-dependent damping.
Kerr-Schild Method and Geodesic Structure in Codimension-2 Brane Black Holes
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abstract
We consider the black hole solutions of five-dimensional gravity with a Gauss-Bonnet term in the bulk and an induced gravity term on a 2-brane of codimension-2. Applying the Kerr-Schild method we derive additional solutions which include charge and angular momentum. To improve our understanding of this geometry we study the geodesic structure of such spacetimes.
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(Quasi-)normal modes of rotating black holes and new solitons in Einstein-Gauss-Bonnet
Scalar probe spectra on new rotating black holes and solitons in 5D Einstein-Gauss-Bonnet gravity give gapped mass towers, real soliton frequencies, and rotation-dependent damping.