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Films minces à base de Si nanostructuré pour des cellules ...

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ˆ the hydrogen reacts with the oxygen species in the plasma which are sputtered<br />

from <strong>Si</strong>O 2 target, leading to the growth of a <strong>Si</strong>-rich suboxi<strong>de</strong> at the substrate.<br />

Consequently, n 1.95eV increases with r H .<br />

(b) Fourier transform infrared spectroscopy<br />

tel-00916300, version 1 - 10 Dec 2013<br />

Figure 3.6 shows the FTIR spectra of the as-grown SRSO samples with varying r H<br />

in Brewster inci<strong>de</strong>nce and in the inset, the normal inci<strong>de</strong>nce spectra. The TO 3 peak<br />

is normalized to unity as in the previous analysis. The variation of LO 3 and TO 3<br />

peak positions with regard to r H are also shown in the inset.<br />

It can be seen from the<br />

Brewster inci<strong>de</strong>nce spectra that<br />

the LO 3 peak intensity <strong>de</strong>creases<br />

with increasing r H . At<br />

r H = 57%, the LO 3 peak becomes<br />

the least intense, and<br />

a peak around 1107 cm −1 is<br />

observed. We also notice an<br />

increase in disor<strong>de</strong>r with r H<br />

from the increasing intensity of<br />

LO 4 -TO 4 in Brewtser inci<strong>de</strong>nce<br />

Figure 3.6: FTIR spectra - Eect of hydrogen rate<br />

on the SRSO lm structure.<br />

spectra and TO 4 peak in normal<br />

inci<strong>de</strong>nce spectra. Traces<br />

of <strong>Si</strong>-H are seen in all the samples<br />

from the Brewster inci<strong>de</strong>nce<br />

spectra.<br />

The <strong>de</strong>creasing LO 3 intensity can be attributed to the increase in <strong>Si</strong> excess and<br />

therefore agglomeration of <strong>Si</strong>-np leading to lower number of interfaces as discussed<br />

in previous section. The increase in <strong>Si</strong> excess with r H also leads to an increase in<br />

structural disor<strong>de</strong>r thereby enhancing the disor<strong>de</strong>r induced mo<strong>de</strong>s. <strong>Si</strong>milar eect<br />

with increasing <strong>Si</strong> excess by increasing RF power <strong>de</strong>nsity on the target has been<br />

observed in our earlier reports [Hijazi 09a]. The huge <strong>de</strong>crease of LO 3 intensity<br />

and a higher enhancement of the LO 4 -TO 4 mo<strong>de</strong> due to <strong>Si</strong> excess may be a possible<br />

reason for the appearance of the peak around 1107 cm −1 . This peak position has also<br />

been reported as interstitial oxygen in <strong>Si</strong> substrates [Kaiser 56, Borghesi 91, Veve 96]<br />

and at <strong>Si</strong>/<strong>Si</strong>O 2 interfaces [Niu 07]. It has been proposed that interstitial oxygen in<br />

<strong>Si</strong> may have a structure similar to fused silica with <strong>Si</strong>-O-<strong>Si</strong> bond angle 100 ° which<br />

would result in a TO <strong>Si</strong>−O stretching vibration around 1107 cm −1 [Kaiser 56] and<br />

68

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