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gure 5.11. It can be seen clearly that the population in the excited state N 3 follows<br />

the pump prole with regularly alternating maxima and minima as suggested before.<br />

5.3.3 Dynamical losses and gain<br />

In the framework of this thesis, it is assumed that the real part of refractive in<strong>de</strong>x<br />

is a constant, while the imaginary part may <strong>de</strong>pend on the absorption and gain<br />

dynamics according to the following equation,<br />

ñ = n(λ) − ik(λ, x) + ig(λ, x) Eqn (5.31)<br />

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

where n(λ) is the real part of refractive in<strong>de</strong>x which we assume to be unchanged<br />

with the absorption dynamics, k(λ, x) accounts for the dynamic losses (absorption)<br />

and g(λ, x) is the dynamic gain (emission).<br />

Gain refers to an increase in the emitted electromagnetic intensity due to energy<br />

transfers within the medium as compared to the inci<strong>de</strong>nt pump. When the gain is<br />

higher than the absorption in the thin lm, we may expect to see emission. In or<strong>de</strong>r<br />

to simulate the gain and losses few assumptions are ma<strong>de</strong>:<br />

ˆ Dynamic losses k(λ, x): The dynamic losses which <strong>de</strong>pend on the population<br />

of emitters, can be expressed using the following equation,<br />

k(λ, x)= σ abs(λ).N 1 (x).λ<br />

Eqn (5.32)<br />

4π<br />

where σ abs is the absorption cross section, and N 1 is the population of emitters<br />

in the ground state.<br />

In or<strong>de</strong>r to estimate the absorption cross section (σ abs ), and to give a shape to<br />

it, Lorentzian functions are used. Therefore σ abs can be represented by,<br />

σ abs = σ abs.max.<br />

1<br />

1 +<br />

(ω 2 ij(abs) −ω2 ) 2<br />

ω 2 ∆ω 2 (abs)<br />

Eqn (5.33)<br />

where σ abs.max is the maximum value of absorption cross sections, ω ij(abs) is the<br />

frequency of absorption between levels i to j, and ∆ω is the width of the Lorentzian<br />

curve of absorption.<br />

The parameters in equation 5.32 are obtained by giving a shape to k(λ, x) by<br />

tting the experimentally obtained k(λ) with lorentzian function in the energy range<br />

of investigation (1.1 - 2.05 eV) of the emission behaviours (Fig. 5.12).<br />

ˆ Dynamic gain g(λ, x) : <strong>Si</strong>milar to dynamic losses, dynamic gain can also be<br />

represented as a function of emission cross section (σ emis ) and the population<br />

of emitters in the excited state (N 3 ) as follows,<br />

150

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