Initial growth of Ba on Ge(001): An STM and DFT study

W. Koczorowski, A. Puchalska, T. Grzela, M. W. Radny, L. Jurczyszyn, S. R. Schofield, R. Czajka, and N. J. Curson
Phys. Rev. B 91, 235319 – Published 29 June 2015

Abstract

An ordered alkaline-earth submonolayer on a clean Si(001) surface provides a template for growth of the atomically sharp, crystalline Si-oxide interface that is ubiquitous in the semiconductor device industry. It has been suggested that submonolayers of Sr or Ba on Ge(001) could play a similar role as on structurally identical Si(001), overcoming known limitations of the Ge(001) substrate such as amorphization of its oxidation layers. In this paper the initial stage of the Ba oxidation process, i.e., adsorption and organization of Ba atoms on the Ge(001) surface as a function of temperature (270770K) for coverage 1.0 monolayer (ML) and 0.150.4ML, is studied using scanning tunneling microscopy (STM) and density functional theory (DFT). Three types of features have been identified on the Ba-covered Ge(001) surface. They originate from isolated Ba adatoms, isolated Ba ad-dimers, and the Ba ad-dimers assembled into short-range, randomly distributed chains that run across the Ge dimer rows. We find from both STM measurements and DFT calculations that the latter is the dominant structure on Ge(001) with increasing coverage.

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  • Received 20 February 2015
  • Revised 20 May 2015

DOI:https://doi.org/10.1103/PhysRevB.91.235319

©2015 American Physical Society

Authors & Affiliations

W. Koczorowski1,2,*, A. Puchalska3, T. Grzela2, M. W. Radny2,4, L. Jurczyszyn3, S. R. Schofield1,5, R. Czajka2, and N. J. Curson1,6

  • 1London Centre for Nanotechnology, University College London, 17-19 Gordon Street, London, United Kingdom
  • 2Institute of Physics, Poznan University of Technology, ul. Piotrowo 3, 60-965 Poznan, Poland
  • 3Institute of Experimental Physics, University of Wroclaw, pl. Maksa Borna 9, 50-204 Wroclaw, Poland
  • 4School of Mathematical and Physical Sciences, The University of Newcastle, Callaghan 2308, Newcastle, Australia
  • 5Department of Physics and Astronomy, UCL, London, WC1E 6BT, United Kingdom
  • 6Department of Electronic and Electrical Engineering, UCL, London, WC1E 7JE, United Kingdom

  • *Corresponding author: wojciech.koczorowski@put.poznan.pl

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Issue

Vol. 91, Iss. 23 — 15 June 2015

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