Parameterizing Dark Energy Models and Study of Finite Time Future Singularities

Figure 1

(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 Linear parameterizations. (g) shows the variation of with . Different colored paths are obtained for different values of D.

(a)

(b)

(c)

(d)

(e)

(f)

(g)