  A review on spatially flat D-dimensional Friedmann-Robertson-Walker (FRW)
model of the universe has been performed. Some standard parameterizations of
the equation of state parameter of the Dark Energy models are proposed and the
possibilities of finite time future singularities are investigated. It is found
that certain types of these singularities may appear by tuning some parameters
appropriately. Moreover, for a scalar field theoretic description of the model,
it was found that the model undergoes bouncing solutions in some favorable
cases.
