Quantum Gravity on
arXiv:hep-th/0203219 · doi:10.1088/0264-9381/19/15/320
Abstract
We study quantum gravity on using the Chern-Simons formulation of three -dimensional gravity. We derive an exact expression for the partition function for quantum gravity on in a Euclidean path integral approach. We show that the topology of the space relevant for studying de Sitter entropy is a solid torus. The quantum fluctuations of de Sitter space are sectors of configurations of point masses taking a {\em discrete} set of values. The partition function gives the correct semi-classical entropy. The sub-leading correction to the entropy is logarithmic in horizon area, with a coefficient -1. We discuss this correction in detail, and show that the sub-leading correction to the entropy from the dS/CFT correspondence agrees with our result. A comparison with the corresponding results for the BTZ black hole is also presented.
10 pages, revtex4, 1 eps figure, published version
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- On the Thermodynamic Geometry of BTZ Black Holes
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- Exploring de Sitter Space and Holography
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- A de Sitter Farey Tail
- Three-dimensional de Sitter horizon thermodynamics
- Deformed CFT on the Stretched dS Horizon
- Keeping matter in the loop in dS quantum gravity
- Gravitational Wilson Lines in 3D de Sitter
- Entropy of Quantum Black Holes
- Universal near-horizon conformal structure and black hole entropy
- Notes on Euclidean de Sitter space
- Big Bangs and Bounces on the Brane
- A New Census of the Universe's Entropy
- Dwelling on de Sitter
- Comments on Quantum Aspects of Three-Dimensional de Sitter Gravity
- Cosmological Implications of Thermodynamic Split Conjecture