Polytropic gas scalar field models of dark energy
arXiv:1206.0647 · doi:10.1007/s10773-013-1558-7
Abstract
In this work we investigate the polytropic gas dark energy model in the non flat universe. We first calculate the evolution of EoS parameter of the model as well as the cosmological evolution of Hubble parameter in the context of polytropic gas dark energy model. Then we reconstruct the dynamics and the potential of the tachyon and K-essence scalar field models according to the evolutionary behavior of polytropic gas model.
18 pages, 6 Figures
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Cited by in corpus (6)
- An effective quintessence field with a power-law potential
- A note on the relations between thermodynamics, energy definitions and Friedmann equations
- Cosmological constraints on polytropic gas model
- Thermodynamic behavior and stability of Polytropic gas
- Thermodynamic descriptions of Polytropic gas and its viscous type as the dark energy candidates
- Polytropic inspired inflation