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The quantum relative entropy of the Schwarzschild black-hole and the area law

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arxiv 2501.09491 v3 pith:D7TISBYL submitted 2025-01-16 gr-qc cond-mat.stat-mechquant-ph

The quantum relative entropy of the Schwarzschild black-hole and the area law

classification gr-qc cond-mat.stat-mechquant-ph
keywords entropyquantumschwarzschildrelativeareagravitymetricblack-hole
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The area law obeyed by the thermodynamic entropy of black holes is one of the fundamental results relating gravity to statistical mechanics. In this work we provide a derivation of the area law for the quantum relative entropy of the Schwarzschild black-hole for arbitrary Schwarzschild radius. The quantum relative entropy between the metric of the manifold and the metric induced by the geometry and the matter field has been proposed in G. Bianconi "Gravity from entropy", Phys. Rev. D (2025) as the action for entropic quantum gravity leading to modified Einstein equations. The quantum relative entropy generalizes Araki entropy and treats the metrics between zero-forms, one-forms, and two-forms as quantum operators. Although the Schwarzschild metric is not an exact solution of the modified Einstein equations of the entropic quantum gravity, it is an approximate solution valid in the low coupling, small curvature limit. Here we show that the quantum relative entropy associated to the Schwarzschild metric obeys the area law for large Schwarzschild radius. We provide a full statistical mechanics interpretation of the results.

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Cited by 2 Pith papers

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