Conserved charges in 3D gravity
arXiv:1003.3782 · doi:10.1103/PhysRevD.81.124024
Abstract
The covariant canonical expression for the conserved charges, proposed by Nester, is tested on several solutions in 3D gravity with or without torsion and topologically massive gravity. In each of these cases, the calculated values of energy-momentum and angular momentum are found to satisfy the first law of black hole thermodynamics.
LATEX, 14 pages; v2: minor corrections, two references added
References in corpus (6)
- Massive Gravity in Three Dimensions
- Warped AdS_3 Black Holes
- Black hole mass and angular momentum in topologically massive gravity
- Asymptotically AdS_3 Solutions to Topologically Massive Gravity at Special Values of the Coupling Constants
- Canonical structure of topologically massive gravity with a cosmological constant
- Stability of warped AdS3 vacua of topologically massive gravity