Chirality dependence of the radial breathing mode: A simple model

Please use this identifier to cite or link to this item: https://physrep.ff.bg.ac.rs/handle/123456789/287

DC Field	Value	Language
dc.contributor.author	Damnjanović, M.	en
dc.contributor.author	Dobardžić, Edib	en
dc.contributor.author	Milošević, I.	en
dc.date.accessioned	2022-07-05T17:30:36Z	-
dc.date.available	2022-07-05T17:30:36Z	-
dc.date.issued	2004-12-15	en
dc.identifier.issn	0953-8984	en
dc.identifier.uri	https://physrep.ff.bg.ac.rs/handle/123456789/287	-
dc.description.abstract	By 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.ispartof	Journal of Physics Condensed Matter	en
dc.title	Chirality dependence of the radial breathing mode: A simple model	en
dc.type	Article	en
dc.identifier.doi	10.1088/0953-8984/16/49/L02	en
dc.identifier.scopus	2-s2.0-10844266652	en
dc.identifier.url	https://api.elsevier.com/content/abstract/scopus_id/10844266652	en
dc.relation.issue	49	en
dc.relation.volume	16	en
item.openairetype	Article	-
item.cerifentitytype	Publications	-
item.fulltext	No Fulltext	-
item.openairecristype	http://purl.org/coar/resource_type/c_18cf	-
item.grantfulltext	none	-
Appears in Collections:	Journal Article

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