English

Interacting cosmic fluids and phase transitions under a holographic modeling for dark energy

General Relativity and Quantum Cosmology 2016-10-12 v1

Abstract

We discuss the consequences of possible sign changes of the QQ-function which measures the energy transference between dark energy and dark matter. We investigate this scenario from a holographic perspective to modeling the dark energy by a linear-parametrization of the equation of state parameter denoted by ω\omega. By imposing the strong constraint of the second law of thermodynamics, we show that sign changes of QQ due to the cosmic evolution imply changes in the temperatures of dark energy and dark matter, respectively. We also discuss the phase transitions, in the past and future, experienced by dark energy and dark matter (or, equivalently, the sign changes of their heat capacities).

Keywords

Cite

@article{arxiv.1511.07186,
  title  = {Interacting cosmic fluids and phase transitions under a holographic modeling for dark energy},
  author = {Samuel Lepe and Francisco Pena},
  journal= {arXiv preprint arXiv:1511.07186},
  year   = {2016}
}