  In this study, we investigate the effects of the one and two-parameters
deformed systems on the Friedmann equations of the Friedmann-Robertson-Walker
(FRW) universe in the context of the entropic gravity approach. We give
simplified forms for the deformed Unruh temperature and Einstein field
equations for three different deformed systems. Based on these compact
equations, we derive the Friedmann equations with the effective gravitational
and cosmological constant.
