| Popis: |
For an FLRW model, thermodynamic phase transitions are investigated in the Einstein-Gauss-Bonnet gravity framework. Using the work density, the equation of state is derived, and the criticality conditions are employed to determine the critical points where possible phase transitions occur. The appearance of phase transitions strongly depends upon the space-time dimension $n$. In this concern, for $n=5$, there is a first-order phase transition, a liquid-gas van der Waals-like phase transition, where the Gibbs free energy presents a swallowtail behavior. On the other hand, for $n=6$, the system does not exhibit a first-order van der Waals-like phase transition. In such a case, the Gibbs free energy presents a cusp with stable and unstable branches. For the present study, the mentioned phenomena are present for an expanding cosmology, where the matter distribution filling the Universe corresponds to a speculative matter distribution with an equation of state parameter greater than one. Interestingly, there are no phase transitions for dimensions higher than $n=6$, nor for expanding or contracting cosmological scenarios. To gain more insights into the system, the micro-structure is analyzed using thermodynamic geometry to quantify the normalized scalar curvature. This invariant shows that a repulsive interaction dominates the phase transition region, while the region where the system has a gas-like behavior attractive interaction prevails. Besides, the critical exponents have been obtained, coinciding their numerical values with the universal ones. |
