Phys. Rev. B 78, 205411 (2008) [9 pages]
Raman signature to identify the structural transition of single-wall carbon nanotubes under high pressure
Abstract
References (31)
Citing Articles
Mingguang Yao, 1 Zhigang Wang, 2,3,4 Bingbing Liu, 1 Yonggang Zou, 1 Shidan Yu, 1 Wang Lin, 1 Yuanyuan Hou, 1 Shoufu Pan, 2,3 Mingxing Jin, 2 Bo Zou, 1 Tian Cui, 1 Guangtian Zou, 1 and B. Sundqvist51State Key Laboratory of Superhard Materials, Jilin University, Changchun 130012, China
2Institute of Atomic and Molecular Physics, Jilin University, Changchun 130012, China
3State Key Laboratory of Theoretical and Computational Chemistry, Institute of Theoretical Chemistry, Jilin University, Changchun 130023, China
4Shanghai Institute of Applied Physics, Chinese Academy of Sciences, P.O. Box 800-204, Shanghai 201800, China
5Department of Physics, Umeå University, 90187 Umeå, Sweden
Received 5 April 2007; revised 28 August 2008; published 10 November 2008
Raman spectra of single-walled carbon nanotubes (SWNTs) with diameters of 0.6–1.3 nm have been studied under high pressure. A “plateau” in the pressure dependence of the G-band frequencies was observed in all experiments, both with and without pressure transmission medium. Near the onset of the G-band plateau, the corresponding radial breathing mode (RBM) lines become very weak. A strong broadening of the full width at half maximum of the RBMs just before the onset of the G-band plateau suggests that a structural transition starts in the SWNTs. Raman spectra from SWNTs released from different pressures also indicate that a significant structural transition occurs during the G-band plateau process. Simulations of the structural changes and the corresponding Raman modes of a nanotube under compression show a behavior similar to the experimental observations. Based on the experimental results and the theoretical simulation, a detailed model is suggested for the structural transition of SWNTs, corresponding to the experimentally obtained Raman results in the high-pressure domain.
©2008 The American Physical Society
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