Cosmic evolution of ghost dark energy models in f(G,T) gravity

The aim of this paper is to study the reconstruction paradigm for both ghost as well as generalized ghost dark energy models in the context of f(G, T) gravity. To accomplish this, we use correspondence scenario for pressureless flat FRW universe with power-law scale factor. The cosmological behavior of reconstructed models is analyzed through graphical analysis of deceleration, equation of state, squared speed of sound parameters and phase planes. It is found that the deceleration parameter represents accelerated epoch for both models whereas equation of state parameter indicates phantom era of the universe for ghost dark energy model and quintessence for its generalized version. The phase planes (omega(eff) - omega(eff)'( )and r - s) indicate the freezing region with phantom phase for both reconstructed dark energy models. We conclude that the squared speed of sound parameter leads to the stability of generalized ghost dark energy model only.