Substrate orientation dependence on the solid phase epitaxial growth rate of Ge
| dc.contributor.author | Darby, B. L. | |
| dc.contributor.author | Yates, B. R. | |
| dc.contributor.author | Martin-Bragado, I. | |
| dc.contributor.author | Gomez-Selles, J. L. | |
| dc.contributor.author | Elliman, R. G. | |
| dc.contributor.author | Jones, K. S. | |
| dc.date.accessioned | 2015-09-21T04:07:47Z | |
| dc.date.available | 2015-09-21T04:07:47Z | |
| dc.date.issued | 2013-01-15 | |
| dc.date.updated | 2016-02-24T08:57:21Z | |
| dc.description.abstract | The 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.sponsorship | The 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.format | 5 pages | |
| dc.identifier.issn | 0021-8979 | en_AU |
| dc.identifier.uri | http://hdl.handle.net/1885/15600 | |
| dc.publisher | American Institute of Physics | |
| dc.rights | http://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.source | Journal of Applied Physics | |
| dc.subject | Keywords: 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.title | Substrate orientation dependence on the solid phase epitaxial growth rate of Ge | |
| dc.type | Journal article | |
| local.bibliographicCitation.issue | 3 | en_AU |
| local.bibliographicCitation.startpage | 033505 | en_AU |
| local.contributor.affiliation | Darby, B.L., University of Florida, United States of America | en_AU |
| local.contributor.affiliation | Yates, B.R., University of Florida, United States of America | en_AU |
| local.contributor.affiliation | Martin-Bragado, I, IMDEA Materials Institute, Spain | en_AU |
| local.contributor.affiliation | Gomez-Selles, J L, IMDEA Materials Institute, Spain | en_AU |
| local.contributor.affiliation | Elliman, Robert, College of Physical and Mathematical Sciences, CPMS Research School of Physics and Engineering, Department of Electronic Materials Engineering, The Australian National University | en_AU |
| local.contributor.affiliation | Jones, K S , University of Florida , United States of America | en_AU |
| local.contributor.authoruid | u9012877 | en_AU |
| local.description.notes | Imported from ARIES | en_AU |
| local.identifier.absfor | 020406 | en_AU |
| local.identifier.absfor | 091205 | en_AU |
| local.identifier.absseo | 970102 | en_AU |
| local.identifier.absseo | 970109 | en_AU |
| local.identifier.absseo | 970110 | en_AU |
| local.identifier.ariespublication | f5625xPUB2379 | en_AU |
| local.identifier.citationvolume | 113 | en_AU |
| local.identifier.doi | 10.1063/1.4776718 | en_AU |
| local.identifier.scopusID | 2-s2.0-84872867083 | |
| local.identifier.thomsonID | 000313670600015 | |
| local.publisher.url | https://www.aip.org/ | en_AU |
| local.type.status | Published Version | en_AU |
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