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
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Cited by in corpus (12)
- Continuous phase transition and critical behaviors of 3D black hole with torsion
- Charged Black Holes in New Massive Gravity
- Phase transition and entropy spectrum of BTZ black hole in three-dimensional gravity with torsion
- Conserved Charges in Extended Theories of Gravity
- Supersymmetric 3D model for gravity with gauge symmetry, mass generation and effective cosmological constant
- Covariant Symplectic Structure and Conserved Charges of Topologically Massive Gravity
- 3D gravity with propagating torsion: the AdS sector
- Conformally flat black holes in Poincaré gauge theory
- 5D Lovelock gravity: new exact solutions with torsion
- Hamiltonian formalism of Minimal Massive Gravity
- Vaidya-like exact solutions with torsion
- Generalizations of the Pontryagin and Husain-Kuchař actions to manifolds with boundary