Thermodynamic properties of modified gravity theories
Kazuharu Bamba

TL;DR
This paper reviews the thermodynamic properties of modified gravity theories like $F(R)$ and $f(T)$ gravity, exploring their thermodynamic equivalences and implications for the universe's second law.
Contribution
It demonstrates the thermodynamic equivalence of equations of motion in modified gravity and explores horizon thermodynamics in both equilibrium and non-equilibrium frameworks.
Findings
Equivalence between modified gravity equations and thermodynamic relations.
Thermodynamics of the cosmological apparent horizon in $f(T)$ gravity.
Second law of thermodynamics holds when horizon temperatures are equal.
Abstract
We review thermodynamic properties of modified gravity theories such as gravity and gravity, where is the scalar curvature and is the torsion scalar in teleparallelism. In particular, we explore the equivalence between the equations of motion for modified gravity theories and the Clausius relation in thermodynamics. In addition, thermodynamics of the cosmological apparent horizon is investigated in gravity. We show both equilibrium and non-equilibrium descriptions of thermodynamics. It is demonstrated that the second law of thermodynamics in the universe can be met when the temperature of the outside of the apparent horizon is equivalent to that of the inside of it.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
