Does horizon entropy satisfy a Quantum Null Energy Conjecture?
Zicao Fu, Donald Marolf

TL;DR
This paper provides evidence that the Hubeny-Rangamani Causal Holographic Information (CHI) satisfies the quantum null energy condition (QNEC) in 1+1 holographic CFTs, supporting its role as a coarse-grained entropy measure in holography.
Contribution
It demonstrates that CHI satisfies the QNEC in specific holographic settings, extending its known properties and supporting its interpretation as a coarse-grained entropy.
Findings
CHI satisfies QNEC in 1+1 holographic CFTs with conical defects in AdS3.
Supports CHI as a meaningful coarse-grained entropy in holography.
Includes derivation of a coarse-grained generalized second law for coupled CFTs and dilaton gravity.
Abstract
A modern version of the idea that the area of event horizons gives times an entropy is the Hubeny-Rangamani Causal Holographic Information (CHI) proposal for holographic field theories. Given a region of a holographic QFTs, CHI computes on a certain cut of an event horizon in the gravitational dual. The result is naturally interpreted as a coarse-grained entropy for the QFT. CHI is known to be finitely greater than the fine-grained Hubeny-Rangamani-Takayanagi (HRT) entropy when lies on a Killing horizon of the QFT spacetime, and in this context satisfies other non-trivial properties expected of an entropy. Here we present evidence that it also satisfies the quantum null energy condition (QNEC), which bounds the second derivative of the entropy of a quantum field theory on one side of a non-expanding null surface by the flux of stress-energy across the…
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