Cosmic acceleration and ekpyrotic bounce with Chameleon field

In this article, we explore the homogeneous and isotropic flat Friedmann-Robertson-Walker (FRW) model in Chameleon cosmology. By considering a non-minimal coupling between scalar field matter, present non-singular bouncing cosmological scenario of universe. The universe initially exhibits ekpyrotic phase during contracting era, undergoes bounce, then expanding it smoothly transits to decelerating era having matter radiation dominated phases. Further, is connected late-time dark energy-dominated epoch. We use numerical solution techniques solve non-minimally coupled gravity equations for understanding evolution along with other quantities like effective potential model. thus unifies an ekpyrotic, non-singular, asymmetric bounce energy study confront observational results on equation state parameter by constraining parameters.