Black hole mass and angular momentum in topologically massive gravity
By A. Bouchareb, G. Clément. 2007
184 citations recorded by the source corpus.
We extend the Abbott–Deser–Tekin approach to the computation of the Killing charge for a solution of topologically massive gravity (TMG) linearized around an arbitrary background. This is then applied to evaluate the mass and angular momentum of black hole solutions of TMG with non-constant curvature asymptotics. The resulting values, together with the appropriate black hole entropy, fit nicely into the first law of black hole thermodynamics.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics, Statistical and Nonlinear Physics
View Paper: https://www.semanticscholar.org/paper/84edb63447b3b41265f6100317e9a609850325a5
How researchers see this paper
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In Astronomy and Astrophysics
- Thomas Hartman
- Andrew Strominger
- A. Maloney
- Dionysios Anninos
- Wei Song
- D. Hofman
- D. Grumiller
- N. Johansson
In Nuclear and High Energy Physics
- Thomas Hartman
- Dionysios Anninos
- Andrew Strominger
- A. Maloney
- Wei Song
- D. Hofman
- D. Grumiller
- N. Johansson
In Statistical and Nonlinear Physics
- Andrew Strominger
- Dionysios Anninos
- A. Maloney
- Wei Song
- Thomas Hartman
- D. Hofman
- D. Grumiller
- N. Johansson
Citations in the corpus
- Warped Conformal Field Theory (2012, methodology): “In this appendix we collect formulae from [77, 78, 32, 35] for the conserved charges in topologically massive gravity.”
- Chiral gravity in three dimensions (2008, background): “Some exact non-Einstein solutions of TMG with arbitrary μ have been found in [30]-[36].”
- Chiral gravity, log gravity, and extremal CFT (2009, background): “(6)This formalism was discussed for general backgrounds in [43], and further generalized in to the case where ξ is not an asymptotic Killing vector [44].”
- Warped AdS3 black holes (2008, background): “1 Metric In [15] a warped black hole closely related to the Schwarzschild solution in 4.”
- Instability in cosmological topologically massive gravity at the chiral point (2008, background): “Since very few exact solutions of CTMG are known [32–37] and because the new mode (3.”