  We have developed an accelerating cosmological model for the present universe
which is phantom for the period $ (0 \leq z \leq 1.99)$ and quintessence phase
for $(1.99 \leq z \leq 2.0315)$. The universe is assumed to be filled with
barotropic and dark energy(DE) perfect fluid in which DE interact with matter.
For a deceleration parameter(DP) having decelerating-accelerating transition
phase of universe, we assume hybrid expansion law for scale factor. The
transition red shift for the model is obtained as $z_t = 0.956$. The model
satisfies current observational constraints.
