A model describing film growth from hyperthermal (1103 eV) species impinging on substrates is presented. The model involves a shallow subsurface implantation process called subplantation, energy loss, preferential displacement of atoms with low displacement energy Ed, leaving the high-Ed atoms intact, sputtering of substrate material, and inclusion of a new phase due to incorporation of a high density of interstitials in a host matrix. Epitaxial or preferred orientation may result from the angular dependence of the Ed and the boundary conditions imposed by the host matrix, i.e., the mold effect. The discussion focuses on deposition of carbon diamondlike films, but examples of other systems, such as Si, Ge, and Ag, are provided as well. The model is supported by classical-ion-trajectory calculations and experimental data. The calculations probe the role of ion range, local concentration, backscattering coefficient, sputtering yield, and ion-induced damage in film evolution. The experimental data emphasize in situ surface-analysis studies of film evolution. The physical parameters of the deposition process that are treated are as follows: (i) nature of bombarding species (C+ versus C-, C- versus C2-, CnHm+, Ar+, and H+), (ii) ion energy, (iii) type of substrate, and (iv) substrate temperature during deposition. © 1990 The American Physical Society.