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It has become apparent that active galactic nuclei (AGN) may have asignificant impact on the growth and evolution of their host galaxies and viceversa but a detailed understanding of the interplay between these processesremains elusive. Deep radio surveys provide a powerful, obscuration-independenttool for measuring both star formation and AGN activity in high-redshiftgalaxies. Multiwavelength studies of deep radio fields show a compositepopulation of star-forming galaxies and AGN, with the former dominating at thelowest flux densities (S$_{1.4\mathrm{GHz}}<$100~$\mu$Jy). The sensitivity andresolution of the SKA will allow us to identify, and separately trace, thetotal star formation in the bulges of individual high-redshift galaxies, therelated nuclear activity and any star formation occurring on larger scaleswithin a disc. We will therefore gain a detailed picture of the apparentlysimultaneous development of stellar populations and black holes in the redshiftrange where both star-formation and AGN activity peak (1$\leq$z$\leq$4). Inthis chapter we discuss the role of the SKA in studying the connection betweenAGN activity and galaxy evolution, and the most critical technical requirementsfor such of studies

The Interplay between SF and AGN Activity, and its role in Galaxy Evolution