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Rotating Gauss-Bonnet BTZ Black Holes

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arxiv 2005.13732 v1 pith:TH6ZP2I6 submitted 2020-05-28 gr-qc hep-th

Robie A. Hennigar , David Kubiznak , Robert B. Mann This is my paper · ORCID
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keywords blackgauss-bonnetrotatinghorizonnovelobtainpropertiessolutions
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We obtain rotating black hole solutions to the novel 3D Gauss-Bonnet theory of gravity recently proposed. These solutions generalize the BTZ metric and are not of constant curvature. They possess an ergoregion and outer horizon, but do not have an inner horizon. We present their basic properties and show that they break the universality of thermodynamics present for their static charged counterparts, whose properties we also discuss. Extending our considerations to higher dimensions, we also obtain novel 4D Gauss-Bonnet rotating black strings.

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Cited by 5 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Spectral Bifurcations in Quasinormal Modes of Regular BTZ Black Holes

    gr-qc 2026-03 conditional novelty 6.0 of 10

    For regular BTZ black holes from an infinite Lovelock tower, scalar quasinormal modes bifurcate from complex BTZ branches into purely imaginary branches as the regularization length ℓ grows, producing mode switching a...

  2. Optimal Control Theory of the (2+1)-Dimensional BTZ Black Hole

    gr-qc 2025-12 conditional novelty 5.0 of 10

    Geodesics of the Weinhold and Ruppeiner thermodynamic metrics are computed for the BTZ black hole and interpreted as optimal evaporation/accretion protocols.

  3. D-dimensional black holes in extended Gauss-Bonnet gravity

    gr-qc 2025-08 conditional novelty 5.0 of 10

    Charged and rotating anti-de Sitter black hole solutions are constructed in extended Gauss-Bonnet gravity for dimensions three, four, five and higher.

  4. Thermodynamics of four-dimensional regular black holes with an infinite tower of regularized curvature corrections

    gr-qc 2025-05 conditional novelty 5.0 of 10

    Planar regular black holes from an infinite tower of higher-curvature corrections are thermodynamically indistinguishable from singular GR black holes, while spherical horizons may lift this degeneracy.

  5. Notes on solution phase space and BTZ black hole

    gr-qc 2024-11 accept novelty 3.0 of 10

    A detailed worked example showing that the solution phase space method reproduces the known mass, angular momentum, entropy, first law, and Smarr relation for the BTZ black hole and three-dimensional Kerr-dS spacetime.

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