Raman resonance window of single-wall carbon nanotubes

J. S. Park, Y. Oyama, R. Saito, W. Izumida, J. Jiang, K. Sato, C. Fantini, A. Jorio, G. Dresselhaus, and M. S. Dresselhaus
Phys. Rev. B 74, 165414 – Published 24 October 2006

Abstract

The spectral width, or γ value, of the Raman excitation profile for single-wall carbon nanotubes is calculated by evaluating the lifetime of the carriers. The calculated results for the γ values are compared with the experimental spectral width of the Raman excitation profile. The γ values evaluated by the electron-phonon interaction show a strong chirality and diameter dependence which is crucial for obtaining the peak intensities of the resonance Raman spectra. Moreover, for metallic carbon nanotubes, we expect an additional contribution to the calculated γ values by comparing them with the experimental results. In particular, we expect that the plasmon excitation in metallic carbon nanotubes may also contribute to the spectral linewidth γ.

    • Received 23 May 2006

    DOI:https://doi.org/10.1103/PhysRevB.74.165414

    ©2006 American Physical Society

    Authors & Affiliations

    J. S. Park1,*, Y. Oyama1, R. Saito1,†, W. Izumida1, J. Jiang1, K. Sato1, C. Fantini2, A. Jorio2, G. Dresselhaus3, and M. S. Dresselhaus4,5

    • 1Department of Physics, Tohoku University and CREST, Sendai, 980-8578, Japan
    • 2Departamento de Física, Universidade Federal de Minas Gerais, Belo Horizonte-MG, 30123-970, Brazil
    • 3Francis Bitter Magnet Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139-4307, USA
    • 4Department of Electrical Engineering and Computer Science, Massachusetts Institute of Technology, Cambridge, Massachussetts 02139-4307, USA
    • 5Department of Physics, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139-4307, USA

    • *Corresponding author. FAX: +81-22-795-6447; Electronic address: park@flex.phys.tohoku.ac.jp
    • Electronic address: rsaito@flex.phys.tohoku.ac.jp

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    Issue

    Vol. 74, Iss. 16 — 15 October 2006

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