Interacting ghost dark energy models with variable G and Λ

In this paper we consider several phenomenological models of variable Lambda. Model of a flat Universe with variable Lambda and G is accepted. It is well known, that varying G and Lambda gives rise to modified field equations and modified conservation laws, which gives rise to many different manipulations and assumptions in literature. We will consider two component fluid, which parameters will enter to Lambda. Interaction between fluids with energy densities rho(1) and rho(2) assumed as Q = 3Hb (rho(1) + rho(2)). We have numerical analyze of important cosmological parameters like EoS parameter of the composed fluid and deceleration parameter q of the model.