Deriving covariant holographic entanglement
Xi Dong, Aitor Lewkowycz, Mukund Rangamani
TL;DR
The paper provides a fully covariant, Lorentzian derivation of the holographic entanglement entropy prescription by embedding the field-theory Schwinger-Keldysh replica construction into the bulk. It shows that, under replica symmetry and appropriate regularity, the dominant bulk saddles in the q→1 limit are governed by codimension-2 extremal surfaces, yielding the HRT area law S_A = Area(E_A)/(4 G_N). The authors thoroughly connect the boundary tracing procedure to bulk geometry via the entanglement wedge and homology constraints, and discuss extensions to higher-derivative gravity, quantum corrections, and potential geometric subtleties such as multiple or complex saddles. This framework clarifies how time-dependent entanglement is encoded holographically and provides a principled route to compute Rényi entropies and modular entropies in dynamical spacetimes.
Abstract
We provide a gravitational argument in favour of the covariant holographic entanglement entropy proposal. In general time-dependent states, the proposal asserts that the entanglement entropy of a region in the boundary field theory is given by a quarter of the area of a bulk extremal surface in Planck units. The main element of our discussion is an implementation of an appropriate Schwinger-Keldysh contour to obtain the reduced density matrix (and its powers) of a given region, as is relevant for the replica construction. We map this contour into the bulk gravitational theory, and argue that the saddle point solutions of these replica geometries lead to a consistent prescription for computing the field theory Renyi entropies. In the limiting case where the replica index is taken to unity, a local analysis suffices to show that these saddles lead to the extremal surfaces of interest. We also comment on various properties of holographic entanglement that follow from this construction.
