Cosmological Entanglement Entropy from the von Neumann Algebra of Double-Scaled SYK & Its Connection with Krylov Complexity
Sergio E. Aguilar-Gutierrez

TL;DR
This paper explores the algebraic entanglement entropy in double-scaled SYK models, connecting it with holographic horizon entropy, Krylov complexity, and the Ryu-Takayanagi formula in (A)dS spaces.
Contribution
It provides a first-principles calculation of holographic entanglement entropy in (A)dS$_2$ space using von Neumann algebras and links it to Krylov complexity.
Findings
Matching algebraic entanglement entropy to Ryu-Takayanagi area in (A)dS$_2$
Reproducing Bekenstein-Hawking and Gibbons-Hawking entropy formulas
Entanglement entropy remains real and depends on Krylov complexity
Abstract
We investigate entanglement entropy between the pair of type II algebras of the double-scaled SYK (DSSYK) model given a chord state, its holographic interpretation as generalized horizon entropy; particularly in the (anti-)de Sitter ((A)dS) space limits of the bulk dual; and its connection with Krylov complexity. The density matrices in this formalism are operators in the algebras, which are specified by the choice of global state; and there exists a trace to evaluate their von Neumann entropy since the algebras are commutants of each other, which leads to a notion of algebraic entanglement entropy. We match it in triple-scaling limits to an area computed through a Ryu-Takayanagi formula in (A)dS space with entangling surfaces at the asymptotic timelike or spacelike boundaries respectively; providing a first-principles example of holographic entanglement entropy for (A)dS…
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