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dc.contributor.authorSHVETS, IGORen
dc.contributor.authorMURPHY, SHANEen
dc.date.accessioned2010-08-12T14:25:20Z
dc.date.available2010-08-12T14:25:20Z
dc.date.issued2007en
dc.date.submitted2007en
dc.identifier.citationChaika, A. N.; Semenov, V. N.; Nazin, S. S..; Bozhko, S. I.; Murphy, S.; Radican, K.; Shvets, I. V., Atomic row doubling in the STM images of Cu(014)-O obtained with MnNi tips, Physical Review Letters, 98, 20, 2007, 206101en
dc.identifier.otherYen
dc.identifier.urihttp://hdl.handle.net/2262/40429
dc.descriptionPUBLISHEDen
dc.description.abstractWe report on scanning tunneling microscopy studies of the Cu(014)-O surface using MnNi tips. Remarkably, the results show a regular apparent doubling of surface atomic rows in the {110} direction. A qualitative explanation of this feature based on tight binding and density functional theory calculations of the electronic structure of the tip is presented. Double imaging of the same atom by different legs of dyz orbital could be the reason for the observed doubling. The orientation of the orbital is determined by the O-Mn crystal field.en
dc.description.sponsorshipThis work was supported by the Russian Academy of Sciences, NT-MDT, RSSF, and FASI grants, Project No. MK-2370.2005.2, Science Foundation Ireland (No. 00/PI.1/C042), and the EU project ASPRINT No. NMP-CT-2003-001601.en
dc.format.extent206101en
dc.language.isoenen
dc.relation.ispartofseriesPhysical Review Lettersen
dc.relation.ispartofseries98en
dc.relation.ispartofseries20en
dc.rightsYen
dc.subjectAtomic, molecular and chemical physicsen
dc.subjectCu(014)-Oen
dc.titleAtomic row doubling in the STM images of Cu(014)-O obtained with MnNi tipsen
dc.typeJournal Articleen
dc.contributor.sponsorScience Foundation Ireland (SFI)en
dc.type.supercollectionscholarly_publicationsen
dc.type.supercollectionrefereed_publicationsen
dc.identifier.peoplefinderurlhttp://people.tcd.ie/ivchvetsen
dc.identifier.peoplefinderurlhttp://people.tcd.ie/shmurphyen
dc.identifier.rssinternalid55198en
dc.identifier.rssurihttp://dx.doi.org/10.1103/PhysRevLett.98.206101en


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