Interacting Ghost Dark Energy Models in the Higher Dimensional Cosmology

Abstract

We investigate interacting ghost dark energy models in higher dimensional cosmology. We attempt to model dark matter within a barotropic fluid with $P_b=\omega (t{)}_b\rho$. In this work we consider four different models based on choosing equation of state parameter and interaction term. We confirm that our models agree with observational data.

13 pages, 6 figures. arXiv admin note: text overlap with arXiv:1308.3450

References in corpus (4)

• Effect of Varying Bulk Viscosity on Generalized Chaplygin Gas
• Latest Observational Constraints to the Ghost Dark Energy Model by Using Markov Chain Monte Carlo Approach
• Phenomenological Varying Modified Chaplygin Gas with Variable $G$ and $\Lambda$: Toy Models for Our Universe
• Interaction between Generalized Varying Chaplygin gas and Tachyonic Fluid