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dc.contributor.authorJorio, A.
dc.contributor.authorSouza Filho, A. G.
dc.contributor.authorBrar, V. W.
dc.contributor.authorSwan, A. K.
dc.contributor.authorÜnlü, M. S.
dc.contributor.authorGoldberg, B. B.
dc.contributor.authorRighi, A.
dc.contributor.authorHafner, J. H.
dc.contributor.authorLieber, C. M.
dc.contributor.authorSaito, R.
dc.contributor.authorDresselhaus, G.
dc.contributor.authorDresselhaus, M. S.
dc.date.accessioned2019-09-27T13:14:36Z
dc.date.issued2002
dc.identifier.citationJorio, A., A. G. Souza Filho, V. W. Brar, A. K. Swan, M. S. Ünlü, B. B. Goldberg, A. Righi, et al. 2002. “Polarized Resonant Raman Study of Isolated Single-Wall Carbon Nanotubes: Symmetry Selection Rules, Dipolar and Multipolar Antenna Effects.” Physical Review B 65 (12). https://doi.org/10.1103/physrevb.65.121402.
dc.identifier.issn1098-0121
dc.identifier.issn1550-235X
dc.identifier.urihttp://nrs.harvard.edu/urn-3:HUL.InstRepos:41417232*
dc.description.abstractWe studied the polarization dependence of the resonance Raman spectra for several different isolated single-wall carbon nanotubes (SWNTs). One isolated SWNT acts as a dipolar antenna, polarized along the tube axis. For light polarized parallel to the tube axis, the strong resonance-effect breaks the symmetry-selection rules, and symmetry-forbidden modes appear in the Raman spectrum. When the light is not polarized parallel to the tube axis, G-band mode symmetries can be identified. Unusual G-mode intensity behavior is observed when the Raman signal is obtained from more than one SWNT, suggesting a complex multipolar antenna pattern.
dc.language.isoen_US
dc.publisherAmerican Physical Society
dash.licenseLAA
dc.titlePolarized resonant Raman study of isolated single-wall carbon nanotubes: Symmetry selection rules, dipolar and multipolar antenna effects
dc.typeJournal Article
dc.description.versionVersion of Record
dc.relation.journalPhysical Review B - Condensed Matter and Materials Physics
dash.depositing.authorLieber, Charles M.::7375001e16c9476d63bde06ba1669b38::600
dc.date.available2019-09-27T13:14:36Z
dash.workflow.comments1Science Serial ID 76338
dc.identifier.doi10.1103/PhysRevB.65.121402
dash.source.volume65;12


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