2006 APS March Meeting 
Monday–Friday, March 13–17, 2006;
Baltimore, MD
Session W18: Focus Session: Carbon Nanotubes: Electronic and Optical Properties III
2:30 PM–5:30 PM, 
Thursday, March 16, 2006
Baltimore Convention Center 
Room: 315
Sponsoring
Unit: 
DMP
Chair: Gordana Dukovic, Columbia University
Abstract ID: BAPS.2006.MAR.W18.1
Abstract: W18.00001 : Phonon sideband in optical spectra of C13 carbon nanotubes
2:30 PM–3:06 PM
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Abstract   
Author:
Shigeo Maruyama
(Dept. of Mech. Eng., The University of Tokyo)
Photoluminescence (PL) of single-walled carbon nanotubes (SWNTs) has been 
widely used for the measurement of chirality distribution of single-walled 
carbon nanotubes (SWNTs). However, there are unassigned peaks in the 2-D 
photoluminescence map plotted as a function of emission and excitation 
photon energy. In order to clarify the origin of these peaks, we have 
studied photoluminescence (PL) and resonant Raman scattering of 
single-walled carbon nanotubes (SWNTs) consisting of carbon-13 
(SW$^{13}$CNTs) synthesized from a small amount of isotopically modified 
ethanol [1]. There was almost no change in the Raman spectra shape for 
SW$^{13}$CNTs except for a downshift of the Raman shift frequency by the 
square-root of the mass ratio 12/13. By comparing photoluminescence 
excitation (PLE) spectra of SW$^{13}$CNTs and normal SWNTs, the excitonic 
phonon sideband due to strong exciton-phonon interaction was clearly 
identified with the expected isotope shift [2]. The PLE line shape and 
energy difference from E$_{ii}$ are remarkably similar to the excitonic 
phonon sideband predicted by Perebeinos \textit{et al.} for (7, 5) and (6, 5) nanotubes. In 
addition to these phonon sideband features, we also found low-intensity 
`pure electronic' features whose origin has never been elucidated. In order 
to examine these `pure electronic' features, polarized PLE measurements on 
individually-dispersed SWNTs aligned in a gelatin-based thin film. By 
comparing optical transitions of SWNTs for incident light parallel or 
perpendicularly polarized to the nanotube axis, we have attributed these 
features to excitation by perpendicularly polarized light to the nanotube 
axis. The measured absorption energies of perpendicularly polarized light 
are compared with cross-polarized version of the Kataura plot.
References:
[1] S. Maruyama and Y. Miyauchi, AIP Conf. Proc. 786, 2005, 100-105.
[2] Y. Miyauchi and S. Maruyama, cond-mat/0508232.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2006.MAR.W18.1