Toward stringy horizons
Elliott Gesteau, Hong Liu
TL;DR
The paper develops a boundary-algebra framework to characterize stringy bulk horizons and quantum extremal surfaces, introducing a causal depth parameter $\mathcal{T}$ and half-sided modular inclusions as diagnostic tools. It shows that above the Hawking–Page temperature, the large $N$ limit of ${\mathcal N}=4$ SYM at finite $\lambda$ exhibits an emergent stringy horizon, while certain toy models do not, and it builds a formalism (ER algebra, modular depth) to discuss connectivity and entropy in the stringy regime. It also connects the horizon/RT/QES questions to spectral data via the exponential type of the boundary spectral function, and discusses potential violations of the bulk equivalence principle, as well as extensions of the ER=EPR program to stringy settings and evaporating black holes. The work points toward a rigorous, algebraic route to stringy bulk geometry, with implications for nonlocality, reconstruction, and the thermodynamics of holographic systems beyond Einstein gravity.
Abstract
We take a first step towards developing a new language to describe causal structure, event horizons, and quantum extremal surfaces (QES) for the bulk description of holographic systems beyond the standard Einstein gravity regime. By considering the structure of boundary operator algebras, we introduce a stringy ``causal depth parameter'', which quantifies the depth of the emergent radial direction in the bulk, and a certain notion of ergodicity on the boundary. We define stringy event horizons in terms of the half-sided inclusion property, which is related to a stronger notion of boundary ergodic or quantum chaotic behavior. Using our definition, we argue that above the Hawking--Page temperature, there is an emergent sharp horizon structure in the large $N$ limit of $\mathcal{N}=4$ Super-Yang--Mills at finite nonzero 't Hooft coupling. In contrast, some previously considered toy models of black hole information loss do not have a stringy horizon. Our methods can also be used to probe violations of the equivalence principle for the bulk gravitational system, and to explore aspects of stringy nonlocality.
