Thermodynamics properties of the dark energy in loop quantum cosmology
Abstract
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. The temperature, chemical potential and entropy are well-defined in the semiclassical regions.
Keywords
Cite
@article{arxiv.1001.0306,
title = {Thermodynamics properties of the dark energy in loop quantum cosmology},
author = {Kui Xiao and Jian-Yang Zhu},
journal= {arXiv preprint arXiv:1001.0306},
year = {2011}
}
Comments
7 pages, no figures, revised version