The $\textrm{T}\bar{\textrm{T}}$ perturbation and its geometric interpretation
Riccardo Conti, Stefano Negro, Roberto Tateo
TL;DR
The paper shows that the classical T T̄ deformation of bosonic 2D theories is equivalent to a spacetime deformation realized by a field-dependent local coordinate change that maps deformed equations of motion to their undeformed counterparts. This is established via a geometric approach rooted in the ZCR/surface formalism, linking TT̄ to JT gravity and yielding a coordinate reparametrization that preserves the intrinsic geometry of solitonic surfaces, notably for the sine-Gordon model where the Gaussian and mean curvatures remain unchanged. The authors extend the construction to N bosons with arbitrary potentials, providing explicit Jacobians that implement the map and revealing how the action acquires a TT̄ (gravitational) contribution under the transformation. Overall, the work bridges classical integrability, differential geometry of embedded surfaces, and holographic interpretations of TT̄, offering a framework to apply integrable-model techniques in TT̄/JT contexts.
Abstract
Starting from the recently-discovered $\textrm{T}\bar{\textrm{T}}$-perturbed Lagrangians, we prove that the deformed solutions to the classical EoMs for bosonic field theories are equivalent to the unperturbed ones but for a specific field-dependent local change of coordinates. This surprising geometric outcome is fully consistent with the identification of $\textrm{T}\bar{\textrm{T}}$-deformed 2D quantum field theories as topological JT gravity coupled to generic matter fields. Although our conclusion is valid for generic interacting potentials, it first emerged from a detailed study of the sine-Gordon model and in particular from the fact that solitonic pseudo-spherical surfaces embedded in $\mathbb R^3$ are left invariant by the deformation. Analytic and numerical results concerning the perturbation of specific sine-Gordon soliton solutions are presented.
