Movement of the spinel-wustite interface in thin films
The wustite-spinel interface boundary can be thought of as a model interface since wustite and spinel share a common f.c.c. oxygen sublattice with only the cations changing across the interface. However, a wide variety of spinel precipitate morphologies has been experimentally observed and ranges from flat plates parallel to {001} planes in the MgAl2O4-MgO system, to coherent ellipsoids parallel to the {001} planes in the NiCr2O4-NiO system, to large coherent particles having “arms” in the <001> direction bounded by {111~ and {110~ planes in the NiFe2O4-NiO system. The particle morphology is determined by a combination of the interfacial energy and the strain energy which results from the lattice misfit between the wustite matrix and the spinel precipitate. In this study, a TEM sample was made containing spinel particles precipitated in the bulk. Individual precipitates were then characterized between a series of anneals.