Thin ceria (CeO2) films were deposited onto a-plane sapphire substrates via
combustion chemical vapor deposition using toluene as a solvent and Ce(III
) 2-ethylhexanoate (Ce-2EH) and tetrakis(2,2,6,6-tetramethyl-3,5-heptanedio
nato)(IV) cerium (Ce-(TMHD)(4)) as chemical precursors. Depositions were ma
de at a substrate temperature of 1000 degrees C using several precursor con
centrations and aerosol size distributions. Ceria assumes the fluorite (cub
ic) structure in the polycrystalline films. Films produced with low concent
rations (similar to 0.001 M) of Ce-2EH display a preferred orientation in w
hich the (200) axis is perpendicular to sapphire substrates. Similar low co
ncentration of Ce-(TMHD)(4) yield films with (111) preferred orientation. H
igh precursor concentrations (>0.002 M) and/or large aerosol size distribut
ions yielded films containing ceria clusters that appear to have nucleated
in the gas phase and adhered to the substrates in addition to material that
nucleated on the substrates. (C) 1999 Elsevier Science Ireland Ltd. All ri
ghts reserved.