  In the background of a flat homogeneous and isotropic space-time, we consider
a scenario of the universe driven by the gravitationally induced `adiabatic'
particle production with constant creation rate. We have shown that this
universe attains a big bang singularity in the past and at late-time it
asymptotically becomes de Sitter. To clarify this model universe, we perform a
dynamical analysis and found that the universe attains a thermodynamic
equilibrium in this late de Sitter phase. Finally, for the first time, we have
discussed the possible effects of `adiabatic' particle creations in the context
of Loop Quantum Cosmology.
