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Main Authors: Barzi, F., Moumni, H. El, Masmar, K.
Format: Preprint
Published: 2025
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Online Access:https://arxiv.org/abs/2509.03470
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author Barzi, F.
Moumni, H. El
Masmar, K.
author_facet Barzi, F.
Moumni, H. El
Masmar, K.
contents We show that Jacobson's thermodynamic derivation of Einstein's equations remains valid when local Rindler horizons are treated as finite heat-capacity systems, resolving the unphysical infinite-bath assumption of standard Unruh thermodynamics. The resulting entropy takes the form of Rényi entropy with nonextensivity parameter $λ\sim C^{-1}$, or equivalently, a new "Einstein entropy" that exactly preserves the Einstein equations for all heat capacities. In both cases, the Unruh temperature is modified as \begin{equation*} T_\text{mod}=\frac{\hbarκ}{2π}\left(1+\frac{S}{C}\right), \end{equation*} establishing a universal link between finite-capacity thermodynamics and nonextensive entropy. We further obtain a corrected scalar Einstein equation with an upper bound on horizon energy flux, pointing to testable signatures in heavy-ion collisions, accelerator spin polarization, and analog gravity experiments. These results reinforce the robustness of the emergent-gravity paradigm and connect spacetime dynamics to generalized entropies of quantum information theory.
format Preprint
id arxiv_https___arxiv_org_abs_2509_03470
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Modified Unruh Thermodynamics in Emergent Gravity: Finite Heat Capacity and Rényi Entropy
Barzi, F.
Moumni, H. El
Masmar, K.
High Energy Physics - Theory
We show that Jacobson's thermodynamic derivation of Einstein's equations remains valid when local Rindler horizons are treated as finite heat-capacity systems, resolving the unphysical infinite-bath assumption of standard Unruh thermodynamics. The resulting entropy takes the form of Rényi entropy with nonextensivity parameter $λ\sim C^{-1}$, or equivalently, a new "Einstein entropy" that exactly preserves the Einstein equations for all heat capacities. In both cases, the Unruh temperature is modified as \begin{equation*} T_\text{mod}=\frac{\hbarκ}{2π}\left(1+\frac{S}{C}\right), \end{equation*} establishing a universal link between finite-capacity thermodynamics and nonextensive entropy. We further obtain a corrected scalar Einstein equation with an upper bound on horizon energy flux, pointing to testable signatures in heavy-ion collisions, accelerator spin polarization, and analog gravity experiments. These results reinforce the robustness of the emergent-gravity paradigm and connect spacetime dynamics to generalized entropies of quantum information theory.
title Modified Unruh Thermodynamics in Emergent Gravity: Finite Heat Capacity and Rényi Entropy
topic High Energy Physics - Theory
url https://arxiv.org/abs/2509.03470