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Modified Unruh thermodynamics in emergent gravity: Finite heat capacity and Rényi entropy

F. Barzi1,2,*, H. El Moumni1,†, and K. Masmar1,‡

  • 1LPTHE, Physics Department, Faculty of Sciences, Ibnou Zohr University, Agadir, Morocco
  • 2CRMEF, Regional Center for Education and Training Professions, Marrakesh, Morocco

  • *Contact author: faical.barzi@edu.uiz.ac.ma
  • †Contact author: h.elmoumni@uiz.ac.ma
  • ‡Contact author: karima.masmar@gmail.com

Phys. Rev. Research 8, 013260 – Published 9 March, 2026

DOI: https://doi.org/10.1103/mnm4-mylh

Abstract

We show that Jacobson's thermodynamic derivation of Einstein's equations remains valid when local Rindler horizons are modeled as finite heat-capacity systems, resolving the infinite-bath assumption of Unruh thermodynamics. The horizon entropy then takes the form of Rényi entropy with nonextensivity parameter λ∼C−1, or equivalently an “Einstein entropy” that uniquely preserves Einstein's equations for arbitrary C. In both cases, the Unruh temperature is modified to Tmod=ℏκ2π1+SC, establishing a universal link between finite-capacity thermodynamics and generalized entropies. We further derive a corrected scalar Einstein equation with an upper bound on horizon energy flux, suggesting testable signatures in heavy-ion collisions, spin-polarization experiments, and analog gravity, emergent gravity.

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