Kaluza-Klein minimally interacting dark energy model in the presence of massive scalar field

In this paper, our purpose is to discuss the dynamical aspects of Kaluza-Klein five-dimensional cosmological model filled with minimally interacting baryonic matter and dark energy (DE) in the presence of an attractive massive scalar field. We obtain a determinate solution of the Einstein field equations using (i) a relation between the metric potentials and (ii) a power law relation between the average scale factor of the universe and the massive scalar field. We have determined scalar field, matter energy density, DE density, equation of state (EoS) (omega <mml:mstyle>de</mml:mstyle>), deceleration (q) and statefinder (r,s) parameters of our model. We also develop omega <mml:mstyle>de</mml:mstyle>-omega <mml:mstyle>de</mml:mstyle>'</mml:msubsup> phase, squared sound speed, statefinders and r-q planes in the evolving universe. It is observed that the EoS parameter exhibits quintom-like behavior from quintessence to phantom epoch by crossing the vacuum era of the universe. The squared speed of sound represents the instability of the model, whereas the <mml:msub>omega <mml:mstyle>de</mml:mstyle>-omega <mml:mstyle>de</mml:mstyle>' plane shows both thawing and freezing regions. The Lambda CDM limit is attained in both r-q and statefinder planes. We have also discussed the cosmological importance of the above parameters with reference to modern cosmology. It is found that the dynamics of these cosmological parameters indicate the accelerated expansion of the universe which is consistent with the current cosmological observations.