Thermodynamics of the FLRW apparent horizon in Einstein-Gauss-Bonnet gravity

TL;DR

This paper investigates the thermodynamic behavior of the apparent horizon in FLRW spacetimes within Einstein-Gauss-Bonnet gravity, revealing how higher-dimensional effects influence thermodynamic variables and suggesting a discretization of the coupling constant.

Contribution

It extends thermodynamic analysis to Einstein-Gauss-Bonnet gravity, incorporating higher-dimensional entropy definitions and exploring the implications for horizon thermodynamics.

Findings

Apparent horizon behaves as a dark energy fluid thermodynamically.

Thermodynamic variables depend on the Gauss-Bonnet coupling and dimension.

Discretization of the Gauss-Bonnet coupling constant is suggested.

Abstract

We analyze the thermodynamic properties of the apparent horizon of Friedmann-Lema\^itre-Roberson-Walker (FLRW) spacetimes in Einstein-Gauss-Bonnet gravity. We use the generalized definition of entropy for gravity theories in higher dimensions to determine the main thermodynamic variables and to compare their behavior with the corresponding quantities in Einstein's theory, emphasizing the role of the Gauss-Bonnet coupling constant and the dimension number. By imposing the validity of the laws of thermodynamics, we show that the apparent horizon can be interpreted thermodynamically as a dark energy fluid, independently of the coupling constant and the dimension number. Using the response functions, we determine the adiabatic index and the number of thermally accesible degrees of freedom of the apparent horizon and argue that this leads to a discretization of the Gauss-Bonnet coupling constant.