Interacting Ghost Dark Energy Models in the Higher Dimensional Cosmology
  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. 
J. Sadeghi, M. Khurshudyan and H. Farahani
gr-qc