On the One-Loop Exactness of Gravity Partition Function
arXiv:2507.16141 · doi:10.1103/r6q6-f79b
Abstract
In a previous work, we showed that the two- and three-loop contributions to the partition function of three-dimensional gravity in flat space vanish. This is in agreement with the expected one-loop exactness dictated by the underlying symmetry at the quantum level. To highlight the distinctive nature of the case, we extend the three-loop computation to arbitrary spacetime dimensions . In higher dimensions, the number of contributions increases substantially, reinforcing the view that one-loop exactness is a unique feature of three-dimensional gravity.
19 pages, 7 figures, 3 tables
References in corpus (13)
- Holographic Reconstruction of Spacetime and Renormalization in the AdS/CFT Correspondence
- New Developments in FeynCalc 9.0
- FeynCalc 9.3: New features and improvements
- Quantum Gravity Partition Functions in Three Dimensions
- Classical central extension for asymptotic symmetries at null infinity in three spacetime dimensions
- One-loop Partition Functions of 3D Gravity
- AdS gravity and random CFT
- A theory of reparameterizations for AdS gravity
- Semiclassical 3D gravity as an average of large-c CFTs
- One-loop partition function of three-dimensional flat gravity
- 3d Quantum Gravity Partition Function at 3 Loops: a brute force computation
- Asymptotic Boundary Conditions and Square Integrability in the Partition Function of AdS Gravity
- One-Loop Partition Function, Gauge Accessibility and Spectra in AdS Gravity