Ni-Al2O3 nanocomposite thin films have been produced on sapphire, sili
con, and silica substrates by a combination of sol-gel processing and
partial reduction reactions. Transmission electron microscopy shows Ni
particles, similar to 20 nm in diameter, embedded in slightly larger
diameter alumina grains. X-ray diffraction lattice parameter measureme
nts suggest that the Ni is in a state of nonhydrostatic strain; Magnet
o-optical Kerr effect measurements indicate that the Ni particles in t
he films on the silicon and silica substrates support perpendicular ma
gnetization. The saturation Kerr rotation increases linearly with film
thickness to values above pure Ni and independent of reflectivity, in
dicating that the material is behaving as a Faraday rotator. The enhan
ced magnetic properties of the composite films are related to the nonh
ydrostatic strain developed in the Ni particles during fabrication. It
is argued that the strains originate from the coefficient of thermal
expansion mismatch between the film and substrate, and likely the volu
me shrinkage associated with the reduction reaction. (C) 1997 American
Institute of Physics.