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This paper derives a first law of proto-area entropy within the CCKLP-Witten holographic framework, establishing a linear relationship between bulk entropy and area variations under specific Gaussian-unitary-ensemble conditions. The analysis identifies a universal response coefficient tied to spectral geometry properties rather than detailed bulk spectrum shapes, offering refined insights into approximate entanglement wedge reconstruction in gravitational scaling limits.
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First Law of Proto-Area Entropy from Modular Spectral Geometry

arXiv2 min read

arXiv:2607.29432v1 Announce Type: cross Abstract: We derive a first law of proto-area entropy in the CCKLP--Witten framework for approximate holographic entanglement wedge reconstruction. The central spectral function admits a modular Hamiltonian representation with kernel $L(x)=x\coth(x/2)$. For near-maximally-mixed bulk states, and within the unstructured Gaussian-unitary-ensemble (GUE) model of the encoding perturbation, the ensemble-averaged proto-area entropy varies linearly with bulk entropy to leading order, with a response coefficient containing a universal factor~$1/3$, traced to $L''(0)/2=1/6$ and independent of the bulk spectrum's detailed shape within this model. Imposing the gravitational-scaling condition required for nonzero backreaction, the first-law coefficient is $O(1)$, parametrically matching the semi-classical relation $\delta({\rm Area}/4G_N)=\delta S_{\rm bulk}$.

Abstract:We derive a first law of proto-area entropy in the CCKLP--Witten framework for approximate holographic entanglement wedge reconstruction. The central spectral function admits a modular Hamiltonian representation with kernel $L(x)=x\coth(x/2)$. For near-maximally-mixed bulk states, and within the unstructured Gaussian-unitary-ensemble (GUE) model of the encoding perturbation, the ensemble-averaged proto-area entropy varies linearly with bulk entropy to leading order, with a response coefficient containing a universal factor~$1/3$, traced to $L''(0)/2=1/6$ and independent of the bulk spectrum's detailed shape within this model. Imposing the gravitational-scaling condition required for nonzero backreaction, the first-law coefficient is $O(1)$, parametrically matching the semi-classical relation $\delta({\rm Area}/4G_N)=\delta S_{\rm bulk}$.

10 pages, 3 figures; submitted to Eur. Phys. J. C

arXiv:2607.29432 [hep-th]

(or arXiv:2607.29432v1 [hep-th] for this version)

https://doi.org/10.48550/arXiv.2607.29432 Focus to learn more arXiv-issued DOI via DataCite (pending registration)

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Full text under the publisher's open licence · 202 words

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