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Substrate orientation dependence on the solid phase epitaxial growth rate of Ge

dc.contributor.authorDarby, B. L.
dc.contributor.authorYates, B. R.
dc.contributor.authorMartin-Bragado, I.
dc.contributor.authorGomez-Selles, J. L.
dc.contributor.authorElliman, R. G.
dc.contributor.authorJones, K. S.
dc.date.accessioned2015-09-21T04:07:47Z
dc.date.available2015-09-21T04:07:47Z
dc.date.issued2013-01-15
dc.date.updated2016-02-24T08:57:21Z
dc.description.abstractThe solid phase epitaxial growth process has been studied at 330 °C by transmission electron microscopy for Ge wafers polished at 10°–15° increments from the [001] to [011] orientations. The velocity showed a strong dependence on substrate orientation with the [001] direction displaying a velocity 16 times greater than the [111] direction. A lattice kinetic Monte Carlo model was used to simulate solid phase epitaxial growth (SPEG) rates at different orientations, and simulations compared well with experimental results. Cross sectional transmission electron microscopy and plan view transmission electron microscopy revealed stacking fault and twin defect formation in the [111] orientation where all other orientations showed only hairpin dislocations. The twin defects formed from Ge SPEG were comparatively less dense than what has previously been reported for Si, which gave rise to higher normalized velocities and a constant [111] SPEG velocity for Ge.
dc.description.sponsorshipThe authors acknowledge Intel Corporation for funding this work. I.M.-B. acknowledges funding from the European project MASTIC (PCIG09-GA-2011-293783).en_AU
dc.format5 pages
dc.identifier.issn0021-8979en_AU
dc.identifier.urihttp://hdl.handle.net/1885/15600
dc.publisherAmerican Institute of Physics
dc.rightshttp://www.sherpa.ac.uk/romeo/issn/0021-8979..."Publishers version/PDF may be used on author's personal website, institutional website or institutional repository" from SHERPA/RoMEO site (as at 21/09/15). Copyright 2013 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 Journal of Applied Physics and may be found at https://doi.org/10.1063/1.4776718
dc.sourceJournal of Applied Physics
dc.subjectKeywords: Cross sectional transmission electron microscopy; Defect formation; Ge wafer; Lattice kinetics; Solid phase epitaxial growth; Substrate orientation; Computer simulation; Defects; Epitaxial growth; Silicon wafers; Transmission electron microscopy; Velocity
dc.titleSubstrate orientation dependence on the solid phase epitaxial growth rate of Ge
dc.typeJournal article
local.bibliographicCitation.issue3en_AU
local.bibliographicCitation.startpage033505en_AU
local.contributor.affiliationDarby, B.L., University of Florida, United States of Americaen_AU
local.contributor.affiliationYates, B.R., University of Florida, United States of Americaen_AU
local.contributor.affiliationMartin-Bragado, I, IMDEA Materials Institute, Spainen_AU
local.contributor.affiliationGomez-Selles, J L, IMDEA Materials Institute, Spainen_AU
local.contributor.affiliationElliman, Robert, College of Physical and Mathematical Sciences, CPMS Research School of Physics and Engineering, Department of Electronic Materials Engineering, The Australian National Universityen_AU
local.contributor.affiliationJones, K S , University of Florida , United States of Americaen_AU
local.contributor.authoruidu9012877en_AU
local.description.notesImported from ARIESen_AU
local.identifier.absfor020406en_AU
local.identifier.absfor091205en_AU
local.identifier.absseo970102en_AU
local.identifier.absseo970109en_AU
local.identifier.absseo970110en_AU
local.identifier.ariespublicationf5625xPUB2379en_AU
local.identifier.citationvolume113en_AU
local.identifier.doi10.1063/1.4776718en_AU
local.identifier.scopusID2-s2.0-84872867083
local.identifier.thomsonID000313670600015
local.publisher.urlhttps://www.aip.org/en_AU
local.type.statusPublished Versionen_AU

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