Parameterizing Dark Energy Models and Study of Finite Time Future Singularities

Figure 6

(a) and (b) (linear), (c) and (d) (CPL), (e) and (f) (JBP), (g) and (h) (ASSS), and (i) and (j) (Efstathiou) show the variation of scale factor ((a), (c), (e), (g), and (i)) and EoS parameter ((b), (d), (f), (h), and (j)) with the variation in cosmic time for the different parameterization models.

(a)

(b)

(c)

(d)

(e)

(f)

(g)

(h)

(i)

(j)