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Gravitational path integral from the $T^2$ deformation

Alexandre Belin, Aitor Lewkowycz, Gabor Sarosi

TL;DR

This work analyzes a $T^2$ deformation of large $N$ CFTs, a higher-dimensional analog of TTbar, showing that the deformation flow is diffusion-like with a kernel given by a Euclidean gravitational path integral in $d{+}1$ dimensions between two Dirichlet boundaries. It establishes a gauge-invariant connection between the deformed partition function $Z^{(\lambda)}$ and the radial Wheeler–DeWitt wavefunction $\\Psi$, and clarifies the role of counterterms and the gravitational path-integral measure, including a Ricci potential that yields the Einstein–Hilbert action. The authors then relate the radial wavefunction to Hartle–Hawking states and discuss York time, the Lorentzian continuation, and a formula linking the extremal-volume of the maximal slice to derivatives of the HH wavefunction, hinting at a complexity=volume-type interpretation. The discussion highlights open issues such as the uniqueness of the flow, the possibility of a fake bulk, and connections to the Freidel kernel in $d=2$, outlining future directions for validating the gravity interpretation of finite-cutoff holography in higher dimensions.

Abstract

We study a $T^2$ deformation of large $N$ conformal field theories, a higher dimensional generalization of the $T\bar T$ deformation. The deformed partition function satisfies a flow equation of the diffusion type. We solve this equation by finding its diffusion kernel, which is given by the Euclidean gravitational path integral in $d+1$ dimensions between two boundaries with Dirichlet boundary conditions for the metric. This is natural given the connection between the flow equation and the Wheeler-DeWitt equation, on which we offer a new perspective by giving a gauge-invariant relation between the deformed partition function and the radial WDW wave function. An interesting output of the flow equation is the gravitational path integral measure which is consistent with a constrained phase space quantization. Finally, we comment on the relation between the radial wave function and the Hartle-Hawking wave functions dual to states in the CFT, and propose a way of obtaining the volume of the maximal slice from the $T^2$ deformation.

Gravitational path integral from the $T^2$ deformation

TL;DR

This work analyzes a deformation of large CFTs, a higher-dimensional analog of TTbar, showing that the deformation flow is diffusion-like with a kernel given by a Euclidean gravitational path integral in dimensions between two Dirichlet boundaries. It establishes a gauge-invariant connection between the deformed partition function and the radial Wheeler–DeWitt wavefunction , and clarifies the role of counterterms and the gravitational path-integral measure, including a Ricci potential that yields the Einstein–Hilbert action. The authors then relate the radial wavefunction to Hartle–Hawking states and discuss York time, the Lorentzian continuation, and a formula linking the extremal-volume of the maximal slice to derivatives of the HH wavefunction, hinting at a complexity=volume-type interpretation. The discussion highlights open issues such as the uniqueness of the flow, the possibility of a fake bulk, and connections to the Freidel kernel in , outlining future directions for validating the gravity interpretation of finite-cutoff holography in higher dimensions.

Abstract

We study a deformation of large conformal field theories, a higher dimensional generalization of the deformation. The deformed partition function satisfies a flow equation of the diffusion type. We solve this equation by finding its diffusion kernel, which is given by the Euclidean gravitational path integral in dimensions between two boundaries with Dirichlet boundary conditions for the metric. This is natural given the connection between the flow equation and the Wheeler-DeWitt equation, on which we offer a new perspective by giving a gauge-invariant relation between the deformed partition function and the radial WDW wave function. An interesting output of the flow equation is the gravitational path integral measure which is consistent with a constrained phase space quantization. Finally, we comment on the relation between the radial wave function and the Hartle-Hawking wave functions dual to states in the CFT, and propose a way of obtaining the volume of the maximal slice from the deformation.

Paper Structure

This paper contains 16 sections, 101 equations, 1 figure.

Figures (1)

  • Figure 1: Three different Dirichlet problems.