Dark energy and future singularity of the universe in Kaluza-Klein space time

The dark energy model with the equation of state (p_{mathit{DE}} = {-} rho_{mathit{DE}} - Arho_{mathit{DE}}^{alpha} ) is studied in Kaluza-Klein space time. The model comprises and provides realization of several types of singularities in different parameter regimes. We discuss the finite-time singularities into four classes and explicitly present the models which give rise to these singularities by assuming the form of the equation of state of dark energy. Also, we discussed the models in terms of the cosmological redshift and some observational parameters.