Research Article

Parameterizing Dark Energy Models and Study of Finite Time Future Singularities

Figure 3

(a), (b), (c), (d), (e), and (f) show the variation of energy density , pressure , EoS parameter , Hubble parameter , potential , and the scalar field with the variation in for the JBP parameterizations. (g) shows the variation of with . Different colored paths are obtained for different values of D.