Please use this identifier to cite or link to this item: https://physrep.ff.bg.ac.rs/handle/123456789/287
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dc.contributor.authorDamnjanović, M.en
dc.contributor.authorDobardžić, Ediben
dc.contributor.authorMilošević, I.en
dc.date.accessioned2022-07-05T17:30:36Z-
dc.date.available2022-07-05T17:30:36Z-
dc.date.issued2004-12-15en
dc.identifier.issn0953-8984en
dc.identifier.urihttps://physrep.ff.bg.ac.rs/handle/123456789/287-
dc.description.abstractBy a simple dynamical model it is shown that the radial breathing mode of single wall carbon nanotubes is not exactly radial: its longitudinal and circumferential components are non-vanishing and both diameter and chirality dependent. However, the radial component is only diameter sensitive; likewise the frequency.en
dc.relation.ispartofJournal of Physics Condensed Matteren
dc.titleChirality dependence of the radial breathing mode: A simple modelen
dc.typeArticleen
dc.identifier.doi10.1088/0953-8984/16/49/L02en
dc.identifier.scopus2-s2.0-10844266652en
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/10844266652en
dc.relation.issue49en
dc.relation.volume16en
item.openairetypeArticle-
item.fulltextNo Fulltext-
item.cerifentitytypePublications-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.grantfulltextnone-
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