Holographic entanglement entropy, Wilson loops, and neural networks

A bstract We apply artificial neural networks to the holographic inverse problem, reconstructing bulk geometry from boundary entanglement entropy by using the Ryu–Takayanagi area functional as a differentiable loss. Validated on the AdS-Schwarzschild background, this approach recovers the blackening factor with maximum absolute error below 3 × 10 −3 across the entire bulk, reproducibly over independent training runs. For finite-density backgrounds like the Gubser–Rocha model, we demonstrate that equal-time strip entanglement entropy determines only the spatial metric. We resolve this exact one-function degeneracy by incorporating holographic Wilson loop data, which couples to the timelike metric. We present a semi-analytical inversion combining Bilson’s and Hashimoto’s formulas, alongside a general three-network variational method minimizing the combined area and Nambu–Goto actions. The neural network achieves maximum relative errors below 0 . 2% for both metric functions without closed-form derivative relations, and accommodates additional holographic observables at the cost of one extra network and loss term.

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Publication Details

Journal
Journal of High Energy Physics
Published
2026-09-04
DOI
https://doi.org/10.1007/jhep09(2026)073
Primary Topic
Black Holes and Theoretical Physics
Type
article
Field-Weighted Citation Impact
0.00
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article

Holographic entanglement entropy, Wilson loops, and neural networks

Veselin G. Filev
Journal of High Energy Physics
Black Holes and Theoretical Physics
article

Holographic entanglement entropy, Wilson loops, and neural networks

Veselin G. Filev
article en

Abstract

A bstract We apply artificial neural networks to the holographic inverse problem, reconstructing bulk geometry from boundary entanglement entropy by using the Ryu–Takayanagi area functional as a differentiable loss. Validated on the AdS-Schwarzschild background, this approach recovers the blackening factor with maximum absolute error below 3 × 10 −3 across the entire bulk, reproducibly over independent training runs. For finite-density backgrounds like the Gubser–Rocha model, we demonstrate that equal-time strip entanglement entropy determines only the spatial metric. We resolve this exact one-function degeneracy by incorporating holographic Wilson loop data, which couples to the timelike metric. We present a semi-analytical inversion combining Bilson’s and Hashimoto’s formulas, alongside a general three-network variational method minimizing the combined area and Nambu–Goto actions. The neural network achieves maximum relative errors below 0 . 2% for both metric functions without closed-form derivative relations, and accommodates additional holographic observables at the cost of one extra network and loss term.

Journal of High Energy PhysicsVol. 2026(9)
Bulgarian Academy of Sciences (BG)
Openalex Percentile: Top 70%
Black Holes and Theoretical Physics
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Holographic entanglement entropy, Wilson loops, and neural networks — Veselin G. Filev · Journal of High Energy Physics (2026) | TGRS Research Map | TGRS