Local quenches, bulk entanglement entropy and a unitary Page curve
Cesar A. Agón, Sagar F. Lokhande, Juan F. Pedraza
TL;DR
This work tests the Faulkner–Faulkner–Faulkner–Faulkner (FLM) prescription for entanglement entropy in a fully time-dependent AdS3/CFT2 setup, using a local quantum quench in the boundary theory and its bulk dual. The authors compute both the area correction and the bulk entanglement entropy correction at order unity, showing that the bulk and boundary calculations match and thereby validating FLM in a dynamical context. They decompose the entanglement entropy into universal (kinematic) and dynamical parts in the CFT, and reproduce these features holographically through geometric and bulk quantum corrections, including a bulk-based Page curve signaling unitary evolution in this toy model of black hole evaporation. The results illuminate how unitarity can persist in semiclassical gravity for simple excitations, connect bulk modular Hamiltonians to CFT data, and provide a concrete framework for exploring quantum corrections to holographic entanglement in time-dependent spacetimes with potential extensions to higher dimensions and more general quench protocols.
Abstract
Quantum corrections to the entanglement entropy of matter fields interacting with dynamical gravity have proven to be very important in the study of the black hole information problem. We consider a one-particle excited state of a massive scalar field infalling in a pure AdS$_3$ geometry and compute these corrections for bulk subregions anchored on the AdS boundary. In the dual CFT$_2$, the state is given by the insertion of a local primary operator and its evolution thereafter. We calculate the area and bulk entanglement entropy corrections at order $\mathcal{O}(N^0)$, both in AdS and its CFT dual. The two calculations match, thus providing a non-trivial check of the FLM formula in a dynamical setting. Further, we observe that the bulk entanglement entropy follows a Page curve. We explain the precise sense in which our setup can be interpreted as a simple model of black hole evaporation and comment on the implications for the information problem.
