paper

Cosmological evolution of equation of state for dark energy in G-essence models

arXiv:1203.2804 · doi:10.1142/S0218271813500235

Abstract

We explore the cosmological evolution of equation of state (EoS) for dark energy in g-essence models, the action of which is described by a function of both the canonical kinetic term of both the scalar and fermionic fields. We examine g-essence models with realizing the crossing of the phantom divide line of as well as the models in which the universe always stays in the non-phantom (quintessence) phase (). In particular, we find an explicit g-essence model with the crossing from the non-phantom phase to the phantom one (). This transition behavior is consistent with the recent observational data analyses.

33 pages, 21 figures, version accepted for publication in Int. J. Mod. Phys. D

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