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CCSD calculations on C₁₄, C₁₈, and C₂₂ carbon clusters

dc.contributor.authorArulmozhiraja, Sundaram
dc.contributor.authorOhno, Takahisa
dc.date.accessioned2015-11-29T23:37:40Z
dc.date.available2015-11-29T23:37:40Z
dc.date.issued2008-03-17
dc.description.abstractThe structure and energetics of the ring isomers of C(4n+2) (n=3-5) carbon clusters were studied by using coupled-cluster singles and doubles excitation theory to overcome the vast differences existing in the literature. The results obtained in the present study clearly indicate that C₁₄, C₁₈, and C₂₂ carbon rings have bond-length and bond-angle alternated acetylenic minimum energy structures. Contrarily, density functional theory calculations were unable to predict these acetylenic-type structures and they ended up with the cumulenic structures. It is found from the coupled-cluster studies that the lowest-energy ring isomer for the first two members of C(4n+2) series is a bond-angle alternated cumulenic D((2n+1)h) symmetry structure while the same for the remaining members is a bond-length and bond-angle alternated C((2n+1)h) symmetry structure. In C(4n+2) carbon rings, Peierls-type distortion, transformation from bond-angle alternated to bond-length alternated minimum energy structures, occurs at C₁₄ carbon ring.en_AU
dc.description.sponsorshipThis study was supported by the RSS21 project and a Grant-in-Aid for Scientific Research No. 17064017 of MEXT, Government of Japan.en_AU
dc.identifier.issn0021-9606en_AU
dc.identifier.urihttp://hdl.handle.net/1885/16903
dc.publisherAmerican Institute of Physics (AIP)en_AU
dc.rightshttp://www.sherpa.ac.uk/romeo/issn/0021-9606..."Publishers version/PDF may be used on author's personal website, institutional website or institutional repository" from SHERPA/RoMEO site (as at 30/11/15). Copyright 2008 American Institute of Physics. This article may be downloaded for personal use only. Any other use requires prior permission of the author and the American Institute of Physics. The following article appeared in The Journal of Chemical Physics and may be found at https://doi.org/10.1063/1.2838200en_AU
dc.sourceThe Journal of Chemical Physicsen_AU
dc.titleCCSD calculations on C₁₄, C₁₈, and C₂₂ carbon clustersen_AU
dc.typeJournal articleen_AU
local.bibliographicCitation.issue11en_AU
local.bibliographicCitation.startpage114301en_AU
local.contributor.affiliationArulmozhiraja, Sundaram, College of Physical and Mathematical Sciences, CPMS Research School of Chemistry, RSC General, The Australian National Universityen_AU
local.contributor.affiliationOhno, Takahisa, National Institute for Materials Science, Japanen_AU
local.contributor.authoruidu4633119en_AU
local.description.notesImported from ARIESen_AU
local.identifier.absfor030701en_AU
local.identifier.ariespublicationU4217927xPUB660en_AU
local.identifier.citationvolume128en_AU
local.identifier.doi10.1063/1.2838200en_AU
local.publisher.urlhttps://www.aip.org/en_AU
local.type.statusPublished Versionen_AU

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