Interacting Quintessence Models of Dark Energy

Abstract

In this paper we consider two models of quintessence scalar fields with different potentials. Interaction with generalized cosmic Chaplygin gas is also investigated. Cosmological parameters are studied and graphical behavior is analyzed. We find that our model is agree with observational data specially $\Lambda$CDM model.

8 pages, accepted in Int. J. Theor. Phys

References in corpus (3)

• Spectra and Light Curves of Six Type Ia Supernovae at 0.511 < z < 1.12 and the Union2 Compilation
• Interacting holographic generalized Chaplygin gas model
• FRW Bulk Viscous Cosmology with Modified Chaplygin Gas in Flat Space

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