Off-shell Partition Functions in 3d Gravity
Lorenz Eberhardt

TL;DR
This paper develops a geometric quantization approach to compute off-shell partition functions in 3d chiral gravity, including cases without classical solutions, and relates these to topological recursion and JT gravity.
Contribution
It introduces a novel method using geometric quantization and equivariant localization to compute off-shell partition functions in 3d gravity, extending to non-classical solutions and connecting to JT gravity.
Findings
Partition functions expressed as integrals over moduli space.
Localization reduces complex integrals to finite-dimensional ones.
Topological recursion computes fake partition functions for arbitrary Riemann surfaces.
Abstract
We explore three-dimensional gravity with negative cosmological constant via canonical quantization. We focus on chiral gravity which is related to a single copy of Chern-Simons theory and is simpler to treat in canonical quantization. Its phase space for an initial value surface is given by the appropriate moduli space of Riemann surfaces. We use geometric quantization to compute partition functions of chiral gravity on three-manifolds of the form , where can have asymptotic boundaries. Most of these topologies do not admit a classical solution and are thus not amenable to a direct semiclassical path integral computation. We use an index theorem that expresses the partition function as an integral of characteristic classes over phase space. In the presence of asymptotic boundaries, we use techniques from…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsBlack Holes and Theoretical Physics · Noncommutative and Quantum Gravity Theories · Cosmology and Gravitation Theories
