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Quasilocal Conserved Charges with a Gravitational Chern-Simons Term

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arxiv 1310.1739 v3 pith:OP5PZ6YG submitted 2013-10-07 hep-th gr-qc

Wontae Kim , Shailesh Kulkarni , Sang-Heon Yi This is my paper · ORCID
classification hep-thgr-qc
keywords chargesconservedformulationgravityquasilocalblackchern-simonsgravitational
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We extend our recent work on the quasilocal formulation of conserved charges to a theory of gravity containing a gravitational Chern-Simons term. As an application of our formulation, we compute the off-shell potential and quasilocal conserved charges of some black holes in three-dimensional topologically massive gravity. Our formulation for conserved charges reproduces very effectively the well-known expressions on conserved charges and the entropy expression of black holes in the topologically massive gravity.

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  1. Extended Near Horizon Symmetries of Extremal BTZ Black Holes in 3D Massive Gravity

    hep-th 2024-12 conditional novelty 6.0 of 10

    Near-horizon extremal BTZ black holes in NMG and TMG carry two Virasoro algebras whose central charges equal their spatial-infinity values.

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