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Measurements

Electron Spin Resonance and Transient Photocurrent ... - JuSER

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Chapter 7: Transient Photocurrent <strong>Measurements</strong><br />

Figure 7.8: Symbols are the normalized photocharge measurements taken on (a) sample<br />

C(V = 0.5 V) and (b) sample D (V = 1 V) at the indicated temperatures. The solid lines<br />

are the corresponding calculations using Eq. 7.4 with the parameters indicated.<br />

due to the absorption depth of the laser, which is 160 nm, about 5% of the charge<br />

is attributed to electron motion 1 and has been subtracted from the transient photocharge.<br />

The portions of these transients at early times close to the electronic<br />

rise-time (t < 5 × 10 −8 s) have been excised, as have the late-time portions where<br />

most holes have been collected. The solid lines in Fig. 7.8 are a fit to the experimental<br />

measurements using the parameters listed in table 7.2. Additionally, the<br />

multiple trapping parameter of a typical a-Si:H sample taken from Dinca et al.<br />

[142] are shown. From the fitting a valence band-tail width of ∆E V = 31 meV for<br />

sample C (∆E V = 32 meV for sample D) was derived, which is much narrower<br />

than the widths of ∆E V = 40−50 meV reported for amorphous silicon [140, 142],<br />

but is still substantially larger than the values as low as 22 meV that are reported<br />

for the conduction band-tail in amorphous silicon [131]. Remarkably, the values<br />

for the band mobility of µ 0 = 1cm 2 /Vs for sample C and µ 0 = 2.3 cm 2 /Vs for<br />

D, are essentially the same as has been reported in amorphous silicon (for both<br />

electrons and holes) [131, 140, 142]. In this context it is interesting to note, that<br />

the attempt to escape frequency ν = 9 × 10 8 s −1 (ν = 5 × 10 9 s −1 ) is approximately<br />

two to three orders of magnitude smaller than values that have been reported for<br />

holes in a-Si:H [140, 142].<br />

7.5 Discussion<br />

Transient photocurrent measurements have been performed on microcrystalline<br />

material prepared under plasma-deposition conditions similar to those where best<br />

solar cell performance can be achieved. As pointed out above, for conventional<br />

1 For a detailed discussion of the topic see section 3.1.4<br />

96

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