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Kerr-Schild Method and Geodesic Structure in Codimension-2 Brane Black Holes

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arxiv 0912.0218 v3 pith:GPWCRTVA submitted 2009-12-01 gr-qc hep-th

Bertha Cuadros-Melgar , Susana Aguilar , Nelson Zamorano This is my paper · ORCID
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keywords blackbranecodimension-2geodesicgravitykerr-schildmethodsolutions
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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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  1. (Quasi-)normal modes of rotating black holes and new solitons in Einstein-Gauss-Bonnet

    hep-th 2024-11 conditional novelty 6.0 of 10

    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.

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