Interacting quintessence dark energy models in Lyra manifold
  In this paper, we consider two-component dark energy models in Lyra manifold. The first component is assumed as a quintessence field while the second model may be a viscous polytropic gas, a viscous Van der Waals gas or a viscous modified Chaplygin gas. We also consider the possibility of interaction between components. By using numerical analysis, we study some cosmological parameters of the models and compare them with observational data. 
M. Khurshudyan, J. Sadeghi, R. Myrzakulov, A. Pasqua, and H. Farahani
gr-qc