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the host <strong>Si</strong>O 2 matrix leading to an increase in n 1.95eV . This method is thus advantageous<br />

than method 1 since by controlling the ratio of power <strong>de</strong>nsities between <strong>Si</strong><br />

and <strong>Si</strong>O 2 it is possible to incorporate higher <strong>Si</strong> excess at a higher r d .<br />

3.3.2 Fourier transorm infrared spectroscopy<br />

Figures 3.8a and 3.8b show the FTIR spectroscopy of the co-sputtered SRSO samples<br />

recor<strong>de</strong>d in Brewster and normal inci<strong>de</strong>nces respectively. In all the spectra the TO 3<br />

peak position is normalized to unity for comparison.<br />

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

(a) Brewster inci<strong>de</strong>nce.<br />

(b) Normal inci<strong>de</strong>nce.<br />

Figure 3.8: FTIR spectra of co-sputtered SRSO in (a) Brewster inci<strong>de</strong>nce and (b) normal<br />

inci<strong>de</strong>nce. The straight line in the normal inci<strong>de</strong>nce spectra helps to witness the shift of<br />

v T O3 and the arrows indicate the 1107 cm −1 peak.<br />

With an increase in P <strong>Si</strong> , the LO 3 peak position shifts from 1220 cm −1 to 1187<br />

cm −1 , in addition to a progressive <strong>de</strong>crease of its intensity. The TO 3 peak position<br />

also shifts towards lower wavenumbers as can be seen from the normal inci<strong>de</strong>nce<br />

spectra. The FTIR spectra with increasing P <strong>Si</strong> show the same behaviour as those<br />

shown when r H was increased. Hence the same explanations as <strong>de</strong>tailed in section<br />

3.2.2 are valid. The only dierence in these spectra as compared to method 1, is<br />

the absence of the <strong>Si</strong>-H peak between 870-890 cm −1 indicating these samples were<br />

fabricated un<strong>de</strong>r a pure Ar plasma. The increased <strong>Si</strong> incorporation as <strong>de</strong>noted by<br />

the high refractive in<strong>de</strong>x with increasing P <strong>Si</strong> can also be seen from the FTIR spectra.<br />

71

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