Quantum minimal surfaces from quantum error correction
Chris Akers, Geoff Penington
TL;DR
This work extends holographic entanglement wedge ideas beyond state-independent codes by introducing state-specific bulk reconstruction and a quantum minimal surface prescription applicable to arbitrary quantum codes. It defines a robust area functional A_B via the Choi–Jamiołkowski state and proves an exact equivalence between complementary state-specific product unitary reconstruction and the holographic entropy formula, with a corresponding one-shot minimality property. The framework accommodates approximate and non-isometric codes, thereby addressing more realistic holographic scenarios (e.g., black hole interiors and the Page curve) and enriching the notion of emergent bulk geometry from boundary entanglement. It also surveys subtleties arising from algebras with centers and discusses extensions toward quantum extremality and future connections to gravitational dynamics.
Abstract
We show that complementary state-specific reconstruction of logical (bulk) operators is equivalent to the existence of a quantum minimal surface prescription for physical (boundary) entropies. This significantly generalizes both sides of an equivalence previously shown by Harlow; in particular, we do not require the entanglement wedge to be the same for all states in the code space. In developing this theorem, we construct an emergent bulk geometry for general quantum codes, defining "areas" associated to arbitrary logical subsystems, and argue that this definition is "functionally unique." We also formalize a definition of bulk reconstruction that we call "state-specific product unitary" reconstruction. This definition captures the quantum error correction (QEC) properties present in holographic codes and has potential independent interest as a very broad generalization of QEC; it includes most traditional versions of QEC as special cases. Our results extend to approximate codes, and even to the "non-isometric codes" that seem to describe the interior of a black hole at late times.
