  The present work deals with a cosmological model having particle creation
mechanism in the framework of irreversible thermodynamics. In the second order
non-equilibrium thermodynamical prescription, the particle creation rate is
treated as the dissipative effect. The non-equilibrium thermodynamical process
is assumed to be isentropic, and, as a consequence, the entropy per particle is
constant, and, hence, the dissipative pressure can be expressed linearly in
terms of the particle creation rate in the background of the homogeneous and
isotropic flat FLRW model. By proper choice of the particle creation rate as a
function of the Hubble parameter, the model shows the evolution of the universe
starting from the inflationary scenario to the present accelerating phase,
considering the cosmic matter as normal perfect fluid with barotropic equation
of state.
