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Introduction to Nanotechnology

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220 OPTICAL AND VIBRATIONAL SPECTROSCOPY<br />

luminescence spectra at various times during the early stages of the emission<br />

process, and the results are presented in Fig. 8.32. The four spectra at the <strong>to</strong>p of<br />

the figure cover the timespan from 0.05 <strong>to</strong> 1 ns, and they demonstrate that there is a<br />

gradual shift of the -556nm spectral line peak <strong>to</strong>ward longer wavelengths during<br />

the first nanosecond of the emission, with the spectral features remaining stable<br />

during the remainder of the decay. The initial extremely fast component of the decay,<br />

for times less than 0.05 ns, arises from resonant emission, and the subsequent fast<br />

component that underwent the wavelength shift A1 - 2 nm shown in Fig. 8.32 was<br />

attributed <strong>to</strong> longitudinal optical (LO) phonon vibrations.<br />

The model sketched in Fig. 8.33 has been proposed <strong>to</strong> explain these results. The<br />

initial 400-nm laser excitation produces electron-hole pairs that either form free<br />

exci<strong>to</strong>ns or become trapped at surface states. Some of the free exci<strong>to</strong>ns decay rapidly<br />

by the emission of a - 1.87-eV pho<strong>to</strong>n, and others quickly become trapped and then<br />

decay almost as rapidly with the emission of a 1.85-eV pho<strong>to</strong>n. The electron-hole<br />

pairs trapped at surface states decay much more slowly, either radiatively by the<br />

emission of pho<strong>to</strong>ns in the range from 1.77 <strong>to</strong> 1.83 eV, or nonradiatively. The rapid<br />

decays occur over a picosecond timescale, and the slower decays over a nanosecond<br />

timescale. This model provides a reasonable explanation of the dynamics of the<br />

nanoparticle luminescence that we have been discussing.<br />

550 555 560 565 570<br />

Wavelength (nm)<br />

Figure 8.32. Time resolved CdS luminescence spectra of the 75cm-’ shift <strong>to</strong>ward longer<br />

wavelengths of the 556-nm line during the first nanosecond after the onset of the emission. The<br />

excitation was at the wavelength I = 549 nm. The intensities of the spectra were adjusted <strong>to</strong><br />

facilitate lineshape comparison. [From M. G. Bawendi, P. J. Carroll, W. L. Wilson, and E. L. Brus,<br />

J. Chern. Phys. 96, 946 (1 992).]

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