Clausius Equation for Horizons in $F(R)$ Gravity
Bohuslav Matou\v{s}

TL;DR
This paper derives thermodynamic properties of horizons in $F(R)$ gravity using a covariant Hamiltonian approach, establishing an analogy with the Clausius equation and comparing results to classical General Relativity.
Contribution
It introduces a covariant Hamiltonian formulation for $F(R)$ gravity to derive horizon temperature and entropy, linking gravitational equations to thermodynamics.
Findings
Horizon temperature and entropy are derived in $F(R)$ gravity.
An analogy between Einstein equations and the Clausius equation is established.
Results are compared with classical General Relativity, highlighting differences and similarities.
Abstract
Covariant Hamiltonian formulation of gravity is used to find variation of surface Hamiltonian which leads to formulation of temperature and entropy of a horizon. These thermodynamic quantities are then used to establish an analogy between Einstein equation and Clausius equation. The obtained results are compared to those from classical General Relativity.
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Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Advanced Thermodynamics and Statistical Mechanics
