2 research outputs found
Monitoring of the Degree of Condensation in Alkoxysiloxane Layers by NIR Reflection Spectroscopy
This
paper introduces a novel analytical approach for monitoring
the degree of condensation of thin siloxane films, which is potentially
suitable for in-line process control during the deposition of such
layers, e.g., to polymer films. Near-infrared (NIR) reflection spectroscopy
in combination with chemometric methods was used as a process monitoring
tool. The state of the formation of the inorganic Si–O–Si
network in partially condensed 3-methacrylÂoxypropylÂtrimethÂoxysilane
batches was analyzed by inverse gated <sup>29</sup>Si NMR spectroscopy.
Results were expressed in terms of different relative ratios of the
T<sup>i</sup> species (i.e., structures with different numbers of
Si–O–Si units per Si atom). These data were used for
calibration of the NIR method, which was applied to thin layers printed
on a polymer foil with a thickness of ∼2.2 g m<sup>–2</sup>. The root-mean-square error of prediction (RMSEP) for the determination
of the ratio of the T<sup>i</sup> species from the NIR spectra was
found to be less than 3%. The error of the reference data from <sup>29</sup>Si NMR spectroscopy is 4%, which results in an overall error
of 5%. Moreover, the thickness of siloxane layers was determined by
this method in a range from 2.5 to 5.5 g m<sup>–2</sup> using
gravimetry for calibration (prediction error ∼0.3 g m<sup>–2</sup>)
Low-Temperature Photochemical Conversion of Organometallic Precursor Layers to Titanium(IV) Oxide Thin Films
Thin
layers of titaniumÂ(IV) ethoxide [TiÂ(OEt)<sub>4</sub>] as a
metal–organic precursor were spin-coated onto silicon wafers
under inert conditions and subsequently photochemically converted
to thin titaniumÂ(IV) oxide (TiO<sub><i>x</i></sub>) films
employing vacuum ultraviolet (VUV) radiation from a xenon excimer
lamp. The photochemical conversion was performed below 35 °C
and at ambient pressure in a nitrogen atmosphere with an optimized
content of oxygen. TiÂ(OEt)<sub>4</sub> decomposition and its kinetics
were monitored and analyzed by gas chromatography and infrared spectroscopy.
Precursor layers with a thickness between 270 and 1060 nm could be
converted into much thinner TiO<sub><i>x</i></sub> films
(40–165 nm). The decrease in thin film thickness was found
to coincide with the removal of organic side chains and densification
to a compact oxide network. For precursor layers with a thickness
of up to 550 nm, VUV irradiation with a moderate radiant exposure
(<i>H</i><sub>e</sub>) of 2.3 J cm<sup>–2</sup> led
to almost carbon-free amorphous layers with a composition close to
stoichiometric titanium dioxide (TiO<sub>2</sub>) having a density
of ∼2.95 g cm<sup>–3</sup> determined by X-ray photoelectron
spectroscopy and X-ray reflectometry, respectively. In turn, crack-free
thin films exhibiting high UV–visible transparency and smooth
surface topography were obtained. The highlighted example of TiÂ(OEt)<sub>4</sub> shows that photochemically initiated decomposition of a metal
alkoxide is a powerful approach for the generation of thin metal oxide
layers at normal pressure and near ambient temperatures