Dynamical analysis of low-energy electron-diffraction intensities from InAs(110)
- 15 May 1983
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review B
- Vol. 27 (10) , 6189-6198
- https://doi.org/10.1103/physrevb.27.6189
Abstract
The measured intensities of 14 diffracted beams of low-energy ( eV) electrons normally incident on InAs(110) are reported. The temperature of the InAs surface during the measurements was K. The surfaces were prepared by ion-bombardment and annealing cycles followed by a verification of surface stochiometry (to within 10%) via Auger electron spectroscopy. Two separate crystals were examined in two separate vacuum instruments in order to verify the reproducibility of the intensity data. The data were analyzed using a relativistic, Hara-exchange electron—ion-core potential and an x-ray -factor structure-analysis methodology. This analysis leads to the best-fit structure of InAs(110) being a rotation of the uppermost layer with the As rotated outward and the In inward. The second layer also is reconstructed with the In being displaced upward by 0.07±0.1 Å relative to its position in the bulk and the As being displaced downward by an equal amount. The x-ray factor for the best-fit structure is . This structure gives a satisfactory visual description of the measured intensities. For bond-length-conserving top-layer rotations the angle between the plane of the surface In-As chains and the plane of truncated bulk surface is , in accordance with expectations based on correlations of covalent radii with prior zinc-blende-structure compound-semiconductor surfaces. The structure of InAs(110) provides the first test of these correlations. The best-fit -factor structure corresponds to reduced relaxation parallel to the surface of the top-layer As relative to that for the bond-length-conserving structure. This best-fit structure is, however, equivalent to its bond-length-conserving counterpart () to within the accuracy of the -factor methodology.
Keywords
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