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Rotating and accelerating AdS black holes in Einstein-Gauss-Bonnet Gravity

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arxiv 2404.04691 v1 pith:M3SH5YV6 submitted 2024-04-06 hep-th gr-qc

Andres Anabalon , Dumitru Astefanesei , Adolfo Cisterna , Fernando Izaurieta , Julio Oliva , Constanza Quijada , Cristian Quinzacara This is my paper · ORCID
classification hep-thgr-qc
keywords rotatingblackrotationacceleratingeinstein-gauss-bonnetholesparametersolutions
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We present new, exact, rotating and accelerating solutions within the framework of five-dimensional Einstein-Gauss-Bonnet theory at the Chern-Simons point. The rotating solutions describe black holes characterized by a single rotation parameter, a mass parameter, and two extra integration constants that can be interpreted as hairs of a gravitational nature. It is noteworthy that the rotation cannot be removed by a large diffeomorphism. We also extend our procedure to dimension seven, providing a new rotating black hole solution with two rotation parameters pertaining to cubic Lovelock theory with a unique vacuum.

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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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