On Holographic Entanglement Density
Nikola I. Gushterov, Andy O'Bannon, Ronnie Rodgers

TL;DR
This paper investigates how holographic entanglement entropy varies with deformations in conformal field theories, revealing insights into states of matter and conditions for area theorem validity or violation.
Contribution
It introduces the concept of entanglement density and analyzes its behavior under various deformations, providing new criteria for characterizing matter states and understanding area theorem violations.
Findings
ED approaches zero from below in Lorentz-invariant RG flows.
ED can approach thermal entropy density from above when Lorentz symmetry is broken.
Small-L behavior of ED is determined by operator dimension or first law of EE.
Abstract
We use holographic duality to study the entanglement entropy (EE) of Conformal Field Theories (CFTs) in various spacetime dimensions , in the presence of various deformations: a relevant Lorentz scalar operator with constant source, a temperature , a chemical potential , a marginal Lorentz scalar operator with source linear in a spatial coordinate, and a circle-compactified spatial direction. We consider EE between a strip or sphere sub-region and the rest of the system, and define the "entanglement density" (ED) as the change in EE due to the deformation, divided by the sub-region's volume. Using the deformed CFTs above, we show how the ED's dependence on the strip width or sphere radius, , is useful for characterizing states of matter. For example, the ED's small- behavior is determined either by the dimension of the perturbing operator or by the first law of EE. For…
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