In this paper, the generalized second law (GSL) of thermodynamics and entropy
is revisited in the context of cosmological models with bouncing behavior such
as chameleon cosmology where the boundary of the universe is assumed to be
enclosed by the dynamical apparent horizon. From a thermodynamic point of view,
to link between thermodynamic and geometric parameters in cosmological models,
we introduce "entropy rate of change multiplied by the temperature" as a model
independent thermodynamic state parameter together with the well known {r,s} statefinder to differentiate the dark energy models.Comment: 11 pages, 5 figures. will be published in Astrophys. Space Sc