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dc.contributor.authorJorio, A.
dc.contributor.authorSaito, R.
dc.contributor.authorHafner, J. H.
dc.contributor.authorLieber, C. M.
dc.contributor.authorHunter, M.
dc.contributor.authorMcClure, T.
dc.contributor.authorDresselhaus, G.
dc.contributor.authorDresselhaus, M. S.
dc.date.accessioned2019-09-27T13:15:47Z
dc.date.issued2001
dc.identifier.citationJorio, A., R. Saito, J. H. Hafner, C. M. Lieber, M. Hunter, T. McClure, G. Dresselhaus, and M. S. Dresselhaus. 2001. “Structural (N,m) Determination of Isolated Single-Wall Carbon Nanotubes by Resonant Raman Scattering.” Physical Review Letters 86 (6): 1118–21. https://doi.org/10.1103/physrevlett.86.1118.
dc.identifier.issn0031-9007
dc.identifier.issn1079-7114
dc.identifier.issn1092-0145
dc.identifier.urihttp://nrs.harvard.edu/urn-3:HUL.InstRepos:41417278*
dc.description.abstractWe show that the Raman scattering technique can give complete structural information for one-dimensional systems, such as carbon nanotubes. Resonant confocal micro-Raman spectroscopy of an (n,m) individual single-wall nanotube makes it possible to assign its chirality uniquely by measuring one radial breathing mode frequency omega (RBM) and using the theory of resonant transitions. A unique chirality assignment can be made for both metallic and semiconducting nanotubes of diameter d(t), using the parameters gamma (0) = 2.9 eV and omega (RBM) = 248/d(t). For example, the strong RBM intensity observed at 156 cm(-1) for 785 nm laser excitation is assigned to the (13, 10) metallic chiral nanotube on a Si/SiO2 surface.
dc.language.isoen_US
dc.publisherAmerican Physical Society
dash.licenseLAA
dc.titleStructural ( n , m ) Determination of Isolated Single-Wall Carbon Nanotubes by Resonant Raman Scattering
dc.typeJournal Article
dc.description.versionVersion of Record
dc.relation.journalPhysical Review Letters
dash.depositing.authorLieber, Charles M.::7375001e16c9476d63bde06ba1669b38::600
dc.date.available2019-09-27T13:15:47Z
dash.workflow.comments1Science Serial ID 78012
dc.identifier.doi10.1103/PhysRevLett.86.1118
dash.source.volume86;6
dash.source.page1118-1121


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