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

on these PL spectra indicate that there is only one low energy peak when the t SRSN<br />

is the lowest (=1.5 nm), and the presence of three peaks is observed for all other<br />

t SRSN .<br />

The peaks are blueshifted with increasing<br />

t SRSN and the positions of peak<br />

(b & c) reach the highest value for the<br />

two highest t SRSN . <strong>Si</strong>milar trend of PL<br />

intensities and peak shifts with varying<br />

Figure 4.38: Inuence of t SRSN on the<br />

PL spectra of SRSO/SRSN ML grown by<br />

reactive sputtering approach, after CA (1h-<br />

1100°C).<br />

t SRSN is observed in MLs with SRSN<br />

grown by co-sputtering approach (not<br />

shown here). This blueshift may indicate<br />

a better connement provi<strong>de</strong>d by<br />

SRSN barriers with increasing t SRSN<br />

thereby preventing overgrowth of <strong>Si</strong>-np<br />

at the interface of SRSO and SRSN sublayers.<br />

The absence of peak (c) for the<br />

lowest t SRSN and the gradually increasing<br />

appearance for higher t SRSN con-<br />

rms the attribution of this peak to<br />

SRSN sublayers. The samples were also subjected to CA to observe the inuence<br />

of t SRSN emission properties after such annealing (Fig. 4.38). The PL after CA<br />

is largely quenched, but t SRSN plays a role in the emission intensity of CA MLs<br />

as well. The increase of PL intensity around 1.5 eV with increasing t SRSN is seen<br />

accompanied by a blueshift of the peak position. <strong>Si</strong>milar to our arguments on STA<br />

emission behaviour, this increase in peak intensity can be attributed to the SRSN<br />

barrier leading to a greater connement of the <strong>Si</strong>-np formed within SRSO, with increasing<br />

t SRSN . Consequently, the size of the <strong>Si</strong>-np <strong>de</strong>creases resulting in a blueshift<br />

and an enhanced emission.<br />

4.9 Optimizing annealing treatments<br />

It has been <strong>de</strong>monstrated in section 4.6 on nitrogen annealing that the SRSO/SRSN<br />

MLs are advantageous over SRSO/<strong>Si</strong>O 2 MLs by achieving higher emission properties<br />

at a lower thermal budget either by using short time annealing at high temperature<br />

(eg. 1min-1000°C [STA]) or longer time at low temperatures (eg. 16min-700°C).<br />

Besi<strong>de</strong>s, a high <strong>de</strong>nsity of <strong>Si</strong>-np is formed after STA resulting in higher absorption<br />

behaviour than SRSO/<strong>Si</strong>O 2 MLs. It has been reported that the passivation of silicon<br />

124

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