Holographic Holes in Higher Dimensions
Robert C. Myers, Junjie Rao, Sotaro Sugishita
TL;DR
This work extends the holographic hole program from AdS$_3$ to higher dimensions and general backgrounds, showing that the Bekenstein-Hawking entropy of bulk surfaces with planar symmetry can be obtained from a boundary differential entropy built from a family of entanglement entropies, with the outer envelope playing a central geometric role. The authors derive the higher-dimensional generalization by analyzing constant-$z$ and varying-$z(x)$ bulk surfaces, extend the construction to Lovelock gravity via the Jacobson-Myers entropy functional, and demonstrate that the differential entropy matches the bulk gravitational entropy in the continuum limit. They also analyze causal holographic information and find that using $ Chi$ in place of $S$ generally fails to reproduce the bulk entropy in higher dimensions due to nonlocal divergences. The results hold in general holographic backgrounds and with generalized entropy functionals, indicating a robust boundary–bulk link for gravitational entropy and providing a framework for understanding holographic reconstruction from boundary entanglement data. The work opens several avenues, including extending beyond planar symmetry, exploring boundary tilings, and clarifying the boundary interpretation of residual entropy.
Abstract
We extend the holographic construction from AdS3 to higher dimensions. In particular, we show that the Bekenstein-Hawking entropy of codimension-two surfaces in the bulk with planar symmetry can be evaluated in terms of the 'differential entropy' in the boundary theory. The differential entropy is a certain quantity constructed from the entanglement entropies associated with a family of regions covering a Cauchy surface in the boundary geometry. We demonstrate that a similar construction based on causal holographic information fails in higher dimensions, as it typically yields divergent results. We also show that our construction extends to holographic backgrounds other than AdS spacetime and can accommodate Lovelock theories of higher curvature gravity.
