Entanglement inequalities, black holes and the architecture of typical states

TL;DR

This paper demonstrates that typical states in large N holographic CFTs have two characteristic length scales, leading to a factorization of degrees of freedom and implications for black hole isolation and entanglement structure.

Contribution

It introduces a holographic framework showing how typical pure states exhibit scale-based factorization and relates this to black hole structure and entanglement inequalities.

Findings

Typical states have UV and IR length scales determined by energy and charges.

Degrees of freedom between these scales effectively factorize.

Black holes can be isolated from the asymptotic region via entanglement wedges.

Abstract

Using holographic realizations of the Araki-Lieb (AL) inequality, we show that typical pure states in large $N$ holographic CFTs possess two characteristic length scales determined solely by energy and conserved charges: a microscopic $L_{\mathrm{UV}}$ and an infrared $L_{\mathrm{IR}} > L_{\mathrm{UV}}$. Degrees of freedom between these scales effectively factorize -- one purifying the ultraviolet (scales $< L_{\mathrm{UV}}$) and the other the infrared sector (scales $> L_{\mathrm{IR}}$). Remarkably, the pure state factor including the ultraviolet sector is determined only by the energy and conserved charges up to exponentially suppressed corrections. Our results imply that all black holes in anti-de Sitter space can be isolated from an asymptotic region, the corona, that is formed by the inclusion of entanglement wedges for which the AL inequality is saturated, and an effective factorization emerges in the buffer region between the corona and the outer horizon. Crucially, we reproduce predictions of the eigenstate thermalization hypothesis and generalize them to rotating thermal ensembles.