Smooth Crossing of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:msub><mml:mi>w</mml:mi><mml:mi>Λ</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mo>−</mml:mo><mml:mn>1</mml:mn></mml:math> Line in a Single Scalar Field Model : Figure 6

]>Smooth Crossing of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:msub><mml:mi>w</mml:mi><mml:mi>Λ</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mo>−</mml:mo><mml:mn>1</mml:mn></mml:math> Line in a Single Scalar Field Model : Figure 6

Figure 6: State parameters

w_{ϕ} (z)

have been plotted against the red-shift parameter

z

(with

f = 0.5, h = 0.68, t_{0} = 13 Gyr

). Smooth double crossing of the Cosmological constant barrier is observed once again for a different initial data

ρ_{m}^{0} \approx 0.77