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Introduction to Nanotechnology

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108 CARBON NANOSTRUCTURES<br />

D-h D-h DZh<br />

1.316<br />

c'c. C<br />

I I c-c-c-c-c-c-c<br />

c 90.4" c<br />

\;/<br />

1.270 1.264 1.280<br />

D3h D-h<br />

c-c-c-c-c<br />

1.271 1.275<br />

/ \<br />

c-c-c-c-c-c-c-c-c<br />

1.269 1.261 1.269 1.283<br />

D-h<br />

c-c-c<br />

I \ 1.24<br />

C<br />

107.1"<br />

\\ I 1.38<br />

c-c-c<br />

c4h<br />

1.290<br />

c-c-c<br />

C C<br />

I \<br />

C<br />

c\ 119.4' /<br />

c,n,c<br />

C<br />

Figure 5.4. Some examples of the structures of small carbon clusters. [With permission from K.<br />

Raghavacari et al., J. Chem. Phys. 87, 2191 (1987).]<br />

the pathway of the light on its way <strong>to</strong> Earth. Scientists study this extinction by<br />

measuring the intensity of light coming from the stars at different wavelengths, that<br />

is, with different colors. When these studies were made, it was noted that there was<br />

an increased extinction or absorption in the ultraviolet region at a wavelength of<br />

220nm (5.6eV), which was attributed <strong>to</strong> light scattered from small particles of<br />

graphite that were believed <strong>to</strong> be present in the regions between the stars. Figure 5.5<br />

shows a plot of this extinction versus the pho<strong>to</strong>n energy. This explanation for the<br />

optical extinction in the 220-nm region has been widely accepted by astronomers.<br />

Donald Huffman of the University of Arizona and Wolfgang Kratschmer of the<br />

Max Planck Institute of Nuclear Physics in Heidelberg were not convinced of this<br />

explanation, and decided <strong>to</strong> study the question further. Their approach was <strong>to</strong><br />

simulate the graphite dust in the labora<strong>to</strong>ry and investigate light transmission<br />

through it. They made smokelike particles by striking an arc between two graphite<br />

electrodes in a helium gas environment, and then condensing the smoke on quartz<br />

glass plates. Various spectroscopic methods such as infrared and Raman spectro-<br />

scopy, which can measure the vibrational frequencies of molecules, were used <strong>to</strong><br />

investigate the condensed graphite. They did indeed obtain the spectral lines known<br />

<strong>to</strong> arise from graphite, but they also observed four additional IR absorption bands<br />

that did not originate from graphite, and they found this very puzzling.<br />

Although a soccer ball-like molecule consisting of 60 carbon a<strong>to</strong>ms with the<br />

chemical formula C60 had been envisioned by theoretical chemists for a number of

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