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.
Authors
- Veselin G. Filev (ORCID: https://orcid.org/0000-0001-5786-6815)
Institutions
- Bulgarian Academy of Sciences (BG)
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