  We investigate the late time acceleration with a Chaplygin type of gas in
spherically symmetric inhomogeneous model. At the early phase we get
Einstien-deSitter type of solution generalised to inhomogeneous spacetime. But
at late stage of the evolution our solutions admit the accelerating nature of
the universe. For a large scale factor our model behaves like a ?CDM model. We
calculate the deceleration parameter for this anisotropic model, which, unlike
its homogeneous counterpart, shows that the flip is not syn- chronous occurring
early at the outer shells. This is in line with other physical processes in any
inhomogeneous models. Depending upon initial conditions our solution also gives
bouncing universe. In the absence of inhomogeneity our solution reduces to
wellknown solutions in homogeneous case. We have also calculated the effective
deceleration parameter in terms of Hubble parameter. The whole situation is
later discussed with the help of wellknown Raychaudhury equation and the
results are compared with the previous case. This work is an extension of our
recent communication where an attempt was made to see if the presence of extra
dimensions and/or inhomogeneity can trigger an inflation in a matter dominated
Lemaitre Tolman Bondi model.
