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two kinds of emitters in SRSO sublayer and one kind of emitter in SRSN sublayers<br />

towards a <strong>de</strong>eper un<strong>de</strong>rstanding.<br />

5.7 Summary<br />

This chapter <strong>de</strong>als with mo<strong>de</strong>ling the pump prole within the thin lm, and emission<br />

from the thin lm. The results obtained can be summarized as follows:<br />

ˆ The pump intensity varies with angle of inci<strong>de</strong>nce. With 45° inci<strong>de</strong>nce of Ar<br />

laser during PL experiments, the pump intensity is lower than that obtained<br />

from normal inci<strong>de</strong>nce.<br />

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

ˆ For a given condition, the position and intensity of the pump varies nonmonotonously<br />

only by varying the thin lm thickness. This is attributed to<br />

the thickness <strong>de</strong>pen<strong>de</strong>nt reections in the lm.<br />

ˆ With increasing losses, the pump intensity <strong>de</strong>creases. The pump prole varies<br />

monotonously with refractive in<strong>de</strong>x.<br />

ˆ Even if the emitters are homogeneously distributed within the thin lm, they<br />

are subjected to a variable pump prole. Consequently, the distribution of<br />

excited emitters follows the pump prole.<br />

ˆ When the dynamic gain exceeds the dynamic losses, emission peak is evi<strong>de</strong>nced<br />

in medium 1.<br />

ˆ The emission spectra varies non-monotonously with thickness, and refractive<br />

in<strong>de</strong>x. Even slight variations of these parameters inuence the shape of the<br />

curves.<br />

ˆ <strong>Si</strong>mulation of SRSO/<strong>Si</strong>O 2 MLs conrms the presence of two kinds of emitters<br />

in SRSO sublayers.<br />

ˆ <strong>Si</strong>mulation of SRSO/SRSN MLs indicates that both SRSO and SRSN sublayers<br />

contain emitters.<br />

ˆ The low energy peak (peak 1) is attributed to the second kind of emitter in<br />

SRSO sublayer.<br />

ˆ The eect of optical cavity is noticed on the emission spectra.<br />

165

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