MASRI, P;
HARKER, AH;
STONEHAM, AM;
(1983)
NATURE AND DIFFUSION OF THE SELF-INTERSTITIAL IN SILICON.
J PHYS C SOLID STATE
, 16
(18)
L613 - L616.
10.1088/0022-3719/16/18/003.
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Abstract
The authors exploit self-consistent, semi-empirical molecular orbital calculations (CNDO) for large silicon clusters to characterise self-interstitials. Hexagonal (I+) and split (100) forms (I- and probably I0) are favoured among the several forms investigated. Possible extended high-temperature forms are not discussed. The results imply Bourgoin-Corbett (1972) athermal diffusion in p-Si and low-activation energy classical motion in n-Si; local excitation enhanced motion is possible, though not verified, but local heating is unlikely. Results agree well with experiment, both for Si and in understanding the different behaviour of silicon and diamond. The energetic advantage of the split form predicted is also supported by the observed split impurity interstitials and unidentified defects, related to the self-interstitial, observed in structures similar to the split (100) form.
Type: | Article |
---|---|
Title: | NATURE AND DIFFUSION OF THE SELF-INTERSTITIAL IN SILICON |
Open access status: | An open access version is available from UCL Discovery |
DOI: | 10.1088/0022-3719/16/18/003 |
Publisher version: | http://dx.doi.org/10.1088/0022-3719/16/18/003 |
Language: | English |
Additional information: | Text made available to UCL Discovery by kind permission of IOP Publishing, 2012 |
UCL classification: | UCL UCL > Provost and Vice Provost Offices UCL > Provost and Vice Provost Offices > UCL BEAMS UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Physics and Astronomy |
URI: | https://discovery.ucl.ac.uk/id/eprint/157073 |
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