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(a) σ emis.max. = 8.78 x 10 −18 m 2 (b) σ emis.max. = 8.78 x 10 −17 m 2<br />

Figure 5.21: <strong>Si</strong>mulating the width and intensity of PL spectra similar to experimental<br />

curve using single emitter and higher emission cross-sections.<br />

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

by increasing the emission cross-section or by <strong>de</strong>creasing the input widths. However<br />

in all these cases, the width of the theoretical spectra is lower than the experimental<br />

one, and all the curves can be tted with a single peak. These results suggest that<br />

the presence of another peak (peak 1) is not from interference or any other optical<br />

eects.<br />

(c) Photoluminescence from double kind of emitters in multilayer conguration<br />

In or<strong>de</strong>r to conrm the presence of two peaks to be a contribution from two kinds<br />

of emitters, simulations were performed using two emitters leading to two peaks<br />

at 1.4 and 1.5 eV in the input. Several trials were ma<strong>de</strong> by varying the emission<br />

cross-section parameters (see Eqn. 5.36), few of which are shown in gure 5.22a.<br />

The <strong>de</strong>tails of the six trials represented in this gure are given in Appendix 2. It<br />

can be seen that the intensity and width of the theoretically obtained spectra from<br />

few of the trials appear to match well with the experimental one. The PL spectra<br />

from trial 3, was chosen for further analysis (Fig. 5.22b).<br />

The inset of gure 5.22b shows a lorentzian curve t performed on the trial 3<br />

simulated curve (obtained with σ em.max = 8.78 x 10 −17 m 2 for both kinds of emitters,<br />

emission peak centers for the two emitters at 1.55 eV and 1.38 eV, with widths 0.29 eV<br />

and 0.14 eV respectively). The results indicate that the broad peak of the simulated<br />

PL curve can be tted with two peaks with positions and width similar to that<br />

of the experimentally obtained one. This tting operation is not straight-forward,<br />

since the thin lm acts as an optical cavity that lters the spectral distribution of<br />

159

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