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Optoelectronics with Carbon Nanotubes

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elax rapidly to lower non-radiative states 19 . Another factor is an array of phonon modes that<br />

exist in SWNTs; phonons can serve as a valuable measurement tool, but they also make it much<br />

more challenging to understand SWNT optoelectronics. Inelastic scattering of phonons is a<br />

decay mechanism that affects EL and PL efficiency very significantly.<br />

3. Phonon modes in SWNTs<br />

Resonance Raman spectroscopy (RRS) has been a standard tool in the optical<br />

investigation of SWNTs since the first observation of a single-tube RRS in 2001 37 . It is also<br />

commonly used in characterization of bulk samples, but the resonance-dependence of Raman<br />

signal intensities complicates the determination of relative abundance of different tubes. There<br />

are several characteristic phonon modes that are observed in SWNTs using this technique.<br />

Figure I-6 shows an example of phonon dispersion that shows the six branches of phonon modes<br />

in SWNTs. Because of the energy-momentum conservation requirement, one can only observe<br />

phonons near the Γ point in the first order, although secondary processes produce additional<br />

observable peaks. Here, we only discuss some commonly observed modes that are relevant to<br />

PL and EL experiments.<br />

The radial breathing mode (RBM) is the lowest vibrational mode observable in RRS,<br />

ranging in wavenumber from only 100 to 400 cm -1 . It originates from the expansion and<br />

contraction in the radial direction of nanotubes perpendicular to the axis, and is therefore<br />

sensitive to the diameter of the tube. The frequency ωRBM is known to be inversely proportional<br />

to the nanotube diameter; the empirical equation ωRBM = 248 cm -1 nm/d is commonly used to<br />

determine the diameter and even the particular (n, m) assignment of SWNTs on a SiO2 substrate,<br />

as long as the diameter is below ~1.8 nm 37 . For larger diameter tubes, too many SWNTs can be<br />

resonant <strong>with</strong> the laser energy used in a given Raman measurement, so the identification of a<br />

particular SWNT species is difficult. On the other hand, it is very unlikely that one can get a<br />

strong enough RBM signal from any given individual SWNT if the excitation energy does not<br />

happen to be in resonance <strong>with</strong> an absorption energy of that specific tube 38 . In addition, larger<br />

diameter tubes have a small ωRBM, so the Raman peak is not easily distinguishable from the laser<br />

excitation line.<br />

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