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Particle-like solutions to topologically massive gravity

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arxiv gr-qc/9404004 v1 pith:MSLVC63Y submitted 1994-04-05 gr-qc hep-th

Gérard Clément This is my paper · ORCID
classification gr-qchep-th
keywords gravitymassivesolutionstopologicallyappliedapproachasymptoticblack
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The solution of topologically massive gravity with cosmological constant is reduced, for space-times with two commuting Killing vectors, to a special-relativistic dynamical problem. This approach is applied to the construction of a class of exact sourceless, horizonless solutions asymptotic to the BTZ extreme black holes.

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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. 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.

  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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