Driven inhomogeneous CFT as a theory in curved space-time

A bstract For two-dimensional conformal field theories (CFTs) driven by evolving background space-time metrics in a closed universe, we present an operator formulation as a driven inhomogeneous CFT. The Hamiltonian of this theory is given by a background space-time dependent smearing of the stress tensor over the spatial slice. Emphasis is placed on the treatment of the curved-space Weyl anomaly, which we show is realized by the difference between Schrödinger and Heisenberg picture Hamiltonians once an appropriate renormalization scheme, the chirally split scheme, is chosen. As a result, the unitary evolution generated by the background metric coincides with that of a Virasoro quantum circuit. To showcase our formalism, we consider the stress tensor one-point function and the entanglement entropy of an interval in both operator and curved-space formulations. We find that these curved-space observables admit a state interpretation only in the chirally split scheme. Finally, we derive the holographic dual of the driven CFT in three-dimensional gravity, extending previous works to arbitrary driving. The holographic dictionary reproduces the stress tensor one-point function and the entanglement entropy in a diffeomorphism invariant scheme.

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Publication Details

Journal
Journal of High Energy Physics
Published
2026-02-26
DOI
https://doi.org/10.1007/jhep02(2026)255
Primary Topic
Black Holes and Theoretical Physics
Type
article
Field-Weighted Citation Impact
0.00

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article

Driven inhomogeneous CFT as a theory in curved space-time

Jani Kastikainen, Tim Schuhmann, Johanna Erdmenger
Journal of High Energy Physics
Black Holes and Theoretical Physics
article

Driven inhomogeneous CFT as a theory in curved space-time

Jani Kastikainen, Tim Schuhmann, Johanna Erdmenger
article en

Abstract

A bstract For two-dimensional conformal field theories (CFTs) driven by evolving background space-time metrics in a closed universe, we present an operator formulation as a driven inhomogeneous CFT. The Hamiltonian of this theory is given by a background space-time dependent smearing of the stress tensor over the spatial slice. Emphasis is placed on the treatment of the curved-space Weyl anomaly, which we show is realized by the difference between Schrödinger and Heisenberg picture Hamiltonians once an appropriate renormalization scheme, the chirally split scheme, is chosen. As a result, the unitary evolution generated by the background metric coincides with that of a Virasoro quantum circuit. To showcase our formalism, we consider the stress tensor one-point function and the entanglement entropy of an interval in both operator and curved-space formulations. We find that these curved-space observables admit a state interpretation only in the chirally split scheme. Finally, we derive the holographic dual of the driven CFT in three-dimensional gravity, extending previous works to arbitrary driving. The holographic dictionary reproduces the stress tensor one-point function and the entanglement entropy in a diffeomorphism invariant scheme.

Journal of High Energy PhysicsVol. 2026(2)
University of Würzburg (DE), Ghent University Hospital (BE)
Deutsche Forschungsgemeinschaft, Fonds Wetenschappelijk Onderzoek, Vlaamse regering
Openalex Percentile: Top 39%
Black Holes and Theoretical Physics
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