Please use this identifier to cite or link to this item: https://doi.org/10.1103/PhysRevB.72.193402
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dc.titleReactive Co magic cluster formation on Si(111)-(7×7)
dc.contributor.authorZilani, M.A.K.
dc.contributor.authorSun, Y.Y.
dc.contributor.authorXu, H.
dc.contributor.authorLiu, L.
dc.contributor.authorFeng, Y.P.
dc.contributor.authorWang, X.-S.
dc.contributor.authorWee, A.T.S.
dc.date.accessioned2014-10-16T09:39:03Z
dc.date.available2014-10-16T09:39:03Z
dc.date.issued2005-11-15
dc.identifier.citationZilani, M.A.K., Sun, Y.Y., Xu, H., Liu, L., Feng, Y.P., Wang, X.-S., Wee, A.T.S. (2005-11-15). Reactive Co magic cluster formation on Si(111)-(7×7). Physical Review B - Condensed Matter and Materials Physics 72 (19) : -. ScholarBank@NUS Repository. https://doi.org/10.1103/PhysRevB.72.193402
dc.identifier.issn10980121
dc.identifier.urihttp://scholarbank.nus.edu.sg/handle/10635/97763
dc.description.abstractCobalt-induced magic clusters have been grown on Si(111)-(7×7). In situ scanning tunneling microscopy studies show that the clusters are off-center in the 7×7 half-unit-cell breaking the local threefold symmetry, and thereby distinguishing this system from other group-III magic clusters. Another unique feature of these clusters is that they are accompanied by voids created by two missing adatoms. Supported by first-principles total energy calculations, we propose a model to explain the atomic structure and formation mechanism of these clusters. The reactive nature of Co leads to the liberation of substrate Si atoms which eventually bond with Co to form the clusters. © 2005 The American Physical Society.
dc.description.urihttp://libproxy1.nus.edu.sg/login?url=http://dx.doi.org/10.1103/PhysRevB.72.193402
dc.sourceScopus
dc.typeArticle
dc.contributor.departmentPHYSICS
dc.description.doi10.1103/PhysRevB.72.193402
dc.description.sourcetitlePhysical Review B - Condensed Matter and Materials Physics
dc.description.volume72
dc.description.issue19
dc.description.page-
dc.description.codenPRBMD
dc.identifier.isiut000233603700023
Appears in Collections:Staff Publications

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