The entropy of bulk quantum fields and the entanglement wedge of an evaporating black hole
Ahmed Almheiri, Netta Engelhardt, Donald Marolf, Henry Maxfield
TL;DR
The paper investigates how bulk quantum fields influence the generalized entropy and the entanglement wedge in evaporating black holes using a two-boundary JT gravity model coupled to a bath. By tracking quantum extremal surfaces through evaporation, it demonstrates a Page-time phase transition and a Hayden-Preskill-like information recovery through a quantum surface that moves away from the classical horizon, consistent with unitarity. The work reveals a rich QES structure, including a novel surface that arises from quantum effects rather than a small perturbation of a classical surface, and analyzes left-right QES gaps in the context of information recovery from the bath. These results provide a holographic realization of information scrambling and recovery in a controlled low-dimensional setting, with implications for higher-dimensional black holes and the interpretation of entanglement wedges in evaporating spacetimes.
Abstract
Bulk quantum fields are often said to contribute to the generalized entropy $\frac{A}{4G_N} +S_{\mathrm{bulk}}$ only at $O(1)$. Nonetheless, in the context of evaporating black holes, $O(1/G_N)$ gradients in $S_{\mathrm{bulk}}$ can arise due to large boosts, introducing a quantum extremal surface far from any classical extremal surface. We examine the effect of such bulk quantum effects on quantum extremal surfaces (QESs) and the resulting entanglement wedge in a simple two-boundary $2d$ bulk system defined by Jackiw-Teitelboim gravity coupled to a 1+1 CFT. Turning on a coupling between one boundary and a further external auxiliary system which functions as a heat sink allows a two-sided otherwise-eternal black hole to evaporate on one side. We find the generalized entropy of the QES to behave as expected from general considerations of unitarity, and in particular that ingoing information disappears from the entanglement wedge after a scambling time $\fracβ{2π} \ln ΔS + O(1)$ in accord with expectations for holographic implementations of the Hayden-Preskill protocol. We also find an interesting QES phase transition at what one might call the Page time for our process.
