Brane cosmology with a van der Waals equation of state
arXiv:gr-qc/0401060 · doi:10.1023/B:GERG.0000022578.70873.6d
Abstract
The evolution of a Universe confined onto a 3-brane embedded in a five-dimensional space-time is investigated where the cosmological fluid on the brane is modeled by the van der Waals equation of state. It is shown that the Universe on the brane evolves in such a manner that three distinct periods concerning its acceleration field are attained: (a) an initial accelerated epoch where the van der Waals fluid behaves like a scalar field with a negative pressure; (b) a past decelerated period which has two contributions, one of them is related to the van der Waals fluid which behaves like a matter field with a positive pressure, whereas the other contribution comes from a term of the Friedmann equation on the brane which is inversely proportional to the scale factor to the fourth power and can be interpreted as a radiation field, and (c) a present accelerated phase due to a cosmological constant on the brane.
9 pages, 2 figures, to be published in General Relativity and Gravitation
References in corpus (3)
Cited by in corpus (16)
- Cosmo-dynamics and dark energy with non-linear equation of state: a quadratic model
- Van der Waals quintessence stars
- Beyond the perfect fluid hypothesis for dark energy equation of state
- Constraining Van der Waals quintessence by observations
- Inflationary universe in terms of a van der Waals viscous fluid
- Cosmological model with non-minimally coupled fermionic field
- Dark energy interacting with neutrinos and dark matter: a phenomenological theory
- Cosmological model involving an interacting van der Waals fluid
- Cosmological evolution with quadratic gravity and nonideal fluids
- The unified history of the viscous accelerating universe and phase transitions
- The van der Waals fluid and its role in cosmology
- Realistic Equations of State for the Primeval Universe
- Thermodynamic analysis for Non-linear system (Van-der-Waals EOS) with viscous cosmology
- Non-Singular Bouncing cosmology from Phantom Scalar-Gauss-Bonnet Coupling: Reconstruction with Observational Insights
- Thermodynamics and energy condition analysis for Van-Der-Waals EOS without viscous cosmology
- The Effects of Spatial Curvature on Cosmic Evolution