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[摘要]：A detailed knowledge of the manifold of both bright and dark excitons in single-walled carbon nanotubes (SWCNTs) is critical to understanding radiative and non-radiative recombination processes. Exciton-phonon coupling opens up additional absorption and emission channels, some of which may "brighten" the sidebands of optically forbidden (dark) excitonic transitions in optical spectra. In this report, we compare C-12 and C-13-labeled SWCNTs that are highly enriched in the (6,5) species to identify both absorptive and emissive vibronic transitions. We find two vibronic sidebands near the bright E-1(11) singlet exciton, one absorptive sideband similar to 200 meV above, and one emissive sideband similar to 140 meV below, the bright singlet exciton. Both sidebands demonstrate a similar to 50 cm(-1) isotope-induced shift, which is commensurate with exciton-phonon coupling involving phonons of A(1) symmetry (D band, omega similar to 1330 cm(-1)). Independent analysis of each sideband indicates that both sidebands arise from the same dark exciton level, which lies at an energy approximately 25 meV above the bright singlet exciton. Our observations support the recent prediction of, and mounting experimental evidence for, the dark K-momentum singlet exciton lying similar to 25 meV (for the (6,5) SWCNT) above the bright Gamma-momentum singlet. This study represents the first use of C-13-labeled SWCNTs highly enriched in a single nanotube species to unequivocally confirm these sidebands as vibronic sidebands of the dark K-momentum singlet exciton. |
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