Twisted sectors in three-dimensional gravity
arXiv:hep-th/9903178 · doi:10.1103/PhysRevD.60.104022
Abstract
Twisted sectors --solutions to the equations of motion with non-trivial monodromies-- of three dimensional Euclidean gravity are studied. We argue that upon quantization this new sector of the theory provides the necessary (and no more) degrees of freedom to account for the Bekenstein-Hawking entropy.
An unnecessary restriction removed. To appear in PRD. Revtex, no figures, 20 pp
References in corpus (12)
- Gauge Theory Correlators from Non-Critical String Theory
- AdS3 Black Holes and a Stringy Exclusion Principle
- Black Hole Entropy from Conformal Field Theory in Any Dimension
- Conformal description of horizon's states
- What We Don't Know about BTZ Black Hole Entropy
- Statistical Entropy and AdS/CFT Correspondence in BTZ Black Holes
- Conformal Field Theory, Geometry, and Entropy
- A note on covariant action integrals in three dimensions
- Embeddings of the Virasoro algebra and black hole entropy
- A Note on Einstein Gravity on AdS and Boundary Conformal Field Theory
- Virasoro Orbits, AdS_3 Quantum Gravity and Entropy
- Thermodynamics and Statistical Mechanics of Induced Liouville Gravity
Cited by in corpus (7)
- Large N Field Theories, String Theory and Gravity
- Conformal Field Theory, (2+1)-Dimensional Gravity, and the BTZ Black Hole
- AdS/CFT correspondence and near-extremal black hole entropy
- Horizon fluff, semi-classical black hole microstates - Log-corrections to BTZ entropy and black hole/particle correspondence
- Three-Dimensional Gravity with Conformal Scalar and Asymptotic Virasoro Algebra
- A Note on Classical String Dynamics on AdS_3
- On Modular Invariance and 3D Gravitational Instantons