Laser ablation deposition of highly oriented yttria stabilized zirconia (YS
Z) films is important for various technological applications and depends cr
itically on the selection of background environment, with low pressure oxyg
en being the most common choice. Here, the spatial-temporal distribution of
YSZ plume chemistry, excitation states, and energy was determined for abla
tions in vacuum, low pressure O-2, and low pressure Ar, using fluorescence
analyses, element specific imaging techniques, and time-of-flight experimen
ts. It was found that an Ar background considerably promotes excitation and
ionization of zirconium during the first 1-3 mu s after the laser strike.
There is much less zirconium excitation in an O-2 background, where a large
fraction of atomic oxygen with a broad spatial distribution was found. ZrO
and YO molecules were observed in both environments. Their highest concent
rations were in the O-2 background, where fluorescence from these molecules
near the substrate lasted for 2-5 mu s. Neutral species in YSZ plumes were
fitted to Maxwellian type velocity distributions with a shifted center of
mass. Kinetic energies derived from the fitted data were reduced by about a
factor of 2 in Ar and O-2 backgrounds compared to in vacuum. This was not
observed for Zr1+ species, which maintained about 100-120 eV mean kinetic e
nergy nearly independently of the background. The ionization of Zr in the p
resence of Ar, the high velocity of ionized Zr atoms relative to the rest o
f the plume, the generation of molecular ZrO, YO, and atomic oxygen in the
presence of O-2 are potentially important for chemistry and structure contr
ol of YSZ films. (C) 2000 American Institute of Physics. [S0021-8979(00)010
14-8].