Dynamics of dark energy and scalar field models in non-flat universe
This paper is devoted to study the effect of different scalar field models under the influence of interacting generalized ghost pilgrim dark energy model in the framework of non-flat FRW universe. For this purpose, we examine the behavior of equation of state and Hubble parameters for two different values of interaction term. Moreover, we consider Lagrangian density of quintessence, tachyon, k-essence and dilaton models to check the consistency of dark energy model with scalar field models. We also evaluate their corresponding potentials and discuss the behavior of kinetic as well as potential energies graphically. We also check the consistency of fractional density of matter and dark energy with Planks 2018.