A $T \bar{T}$ Deformation for Curved Spacetimes from 3d Gravity
Edward A. Mazenc, Vasudev Shyam, Ronak M Soni

TL;DR
This paper extends the $T ar{T}$ deformation to curved spacetimes by formulating a flow equation for the partition function, linking it to 3d quantum gravity and the Wheeler-de Witt equation, with implications for holography and boundary conditions.
Contribution
It introduces a generalized $T ar{T}$ deformation applicable to curved spaces, connecting deformed CFT partition functions to 3d gravity path integrals and local Wheeler-de Witt equations.
Findings
Deformed partition function solves a local Wheeler-de Witt equation.
Partition function corresponds to a 3d gravity path integral.
Reproduces known flat space and large $c$ results.
Abstract
We propose a generalisation of the deformation to curved spaces by defining, and solving, a suitable flow equation for the partition function. We provide evidence it is well-defined at the quantum level. This proposal identifies, for any CFT, the deformed partition function and a certain wavefunction of 3d quantum gravity. This connection, true for any , is not a holographic duality --- the 3d theory is a "fake bulk." We however emphasise that this reduces to the known holographic connection in the classical limit. Concretely, this means the deformed partition function solves exactly not just one global equation, defining the flow, but in fact a local Wheeler-de Witt equation, relating the operator to the trace of the stress tensor. This also immediately suggests a version of the deformation with locally varying deformation…
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Noncommutative and Quantum Gravity Theories · Cosmology and Gravitation Theories
