Holography For a De Sitter-Esque Geometry
arXiv:1102.3178 · doi:10.1007/JHEP05(2011)003
Abstract
Warped dS arises as a solution to topologically massive gravity (TMG) with positive cosmological constant and Chern-Simons coefficient in the region . It is given by a real line fibration over two-dimensional de Sitter space and is equivalent to the rotating Nariai geometry at fixed polar angle. We study the thermodynamic and asymptotic structure of a family of geometries with warped dS asymptotics. Interestingly, these solutions have both a cosmological horizon and an internal one, and their entropy is unbounded from above unlike black holes in regular de Sitter space. The asymptotic symmetry group resides at future infinity and is given by a semi-direct product of a Virasoro algebra and a current algebra. The right moving central charge vanishes when . We discuss the possible holographic interpretation of these de Sitter-esque spacetimes.
22 pages, 1 figure; v2: typos corrected, to match with published version
References in corpus (18)
- Three-Dimensional Gravity Revisited
- Warped AdS_3 Black Holes
- More on Massive 3D Gravity
- Surface charge algebra in gauge theories and thermodynamic integrability
- Black hole mass and angular momentum in topologically massive gravity
- Three-dimensional black holes, gravitational solitons, kinks and wormholes for BHT massive gravity
- Universal Area Product Formulae for Rotating and Charged Black Holes in Four and Higher Dimensions
- Semi-classical central charge in topologically massive gravity
- Black Hole Entropy in the presence of Chern-Simons Terms
- Measurement of the charm fragmentation function in D* photoproduction at HERA
- Boundary conditions for spacelike and timelike warped AdS_3 spaces in topologically massive gravity
- Micromanaging de Sitter holography
- Asymptotic Symmetries and Charges in De Sitter Space
- Stability of warped AdS3 vacua of topologically massive gravity
- The Curious Case of Null Warped Space
- Self-Dual Warped AdS Black Holes
- All stationary axi-symmetric local solutions of topologically massive gravity
- An introduction to the mechanics of black holes
Cited by in corpus (22)
- Warped Conformal Field Theory
- De Sitter Musings
- Infrared Realization of dS in AdS
- Inner Mechanics of 3d Black Holes
- Thermodynamics of Black Hole Horizons and Kerr/CFT Correspondence
- Higher Spin Realization of the dS/CFT Correspondence
- Holographic perfect fluidity, Cotton energy-momentum duality and transport properties
- Future Boundary Conditions in De Sitter Space
- Incompressible Fluids of the de Sitter Horizon and Beyond
- Warped Symmetries of the Kerr Black Hole
- Quantum Kerr-de Sitter black holes in three dimensions
- Warped AdS_3 Black Holes in Higher Derivative Gravity Theories
- Quantum Topologically Massive Gravity in de Sitter Space
- Quasinormal Modes and Hidden Conformal Symmetry of Warped dS Black Hole
- Asymptotic Symmetries of Three-Dimensional Black Strings
- Warped Flatland
- Gravitational duality, topologically massive gravity and holographic fluids
- Homogeneous anisotropic solutions of topologically massive gravity with cosmological constant and their homogeneous deformations
- Warped Conformal Symmetries of the Accelerating Kerr Black Hole
- Warped CFT duals of the Plebański-Demiański family of solutions
- Gravitational radiations of Kerr black hole from warped symmetries
- Notes on Self-dual Warped dS Spacetime