Quadratic interaction effect on the dark energy density in the universe
Deveci Derya G1, 2, Aydiner Ekrem1, †
       

(color online) (a) The evolution behavior of the effective equations of state (blue) and (red) versus x where x = ln(a/a0) and (b) the evolution behaviors of the density parameters of ΩDE (blue) and Ωk (red) versus x are represented for the non-flat universe (open case) in the case of quadratic EoS with the parameters b2 = 0.1, for an interaction of n = 1 with the initial conditions ΩDE(0) = 0.72, Ωk(0) = 0.08 for k = 1.