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Three-dimensional Chern-Simons black holes

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arxiv 0807.4241 v1 pith:3TZJVN4P submitted 2008-07-26 gr-qc hep-th

K. Ait Moussa , G. Clement , H. Guennoune , C. Leygnac This is my paper · ORCID
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keywords blackchern-simonsholeholeslocalsolutionsthree-dimensionaladmit
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abstract

We construct black hole solutions to three-dimensional Einstein-Maxwell theory with both gravitational and electromagnetic Chern-Simons terms. These intrinsically rotating solutions are geodesically complete, and causally regular within a certain parameter range. Their mass, angular momentum and entropy are found to satisfy the first law of black hole thermodynamics. These Chern-Simons black holes admit a four-parameter local isometry algebra, which generically is $sl(2,R)\times R$, and may be generated from the corresponding vacua by local coordinate transformations.

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Cited by 2 Pith papers

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

  1. 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.

  2. Note on WAdS$_3$ black holes in extended BHT gravity

    hep-th 2024-11 conditional novelty 3.0 of 10

    Using Wald's formalism and the thermodynamics method, the paper computes conserved charges and dual CFT central charges for WAdS3 black holes in NMG and ENMG, finding results consistent with earlier work.

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