Thermodynamics properties of the dark energy in loop quantum cosmology

Understand

Considering an arbitrary, varying equation of the state parameter, the thermodynamic properties of the dark energy fluid in a semiclassical loop quantum cosmology scenario, which we consider the inverse volume modification, is studied.

• The equation of the state parameters are corrected as a semiclassical one during considering the effective behavior.
• Assuming that the apparent horizon has Hawking temperature, the modified entropy-area relation is obtained, we find that this relation is different from the one which is obtained by considering the holonomy correction.
• Considering the dark energy is a thermal equilibrium fluid, we get the expressions for modified temperature, chemical potential and entropy.