We consider a five-dimensional Ricci flat Bouncing cosmology and assume that the four-dimensional universe is permeated smoothly by three minimally coupled matter components : CDM+baryons \rho _ { m } , radiation \rho _ { r } and dark energy \rho _ { x } .
Evolutions of these three components are studied and it is found that dark energy dominates before the bounce , and pulls the universe contracting .
In this process , dark energy decreases while radiation and the matter increase .
After the bounce , the radiation and matter dominates alternatively and then decrease with the expansion of the universe .
At present , the dark energy dominates again and pushes the universe accelerating .
In this model , we also obtain that the equation of state ( EOS ) of dark energy at present time is w _ { x 0 } \approx - 1.05 and the redshift of the transition from decelerated expansion to accelerated expansion is z _ { T } \approx 0.37 , which are compatible with the current observations .