| Parameter | Value | Source |
| a |
5.387(10 |
calculated |
| -5.971 eV/atom | calculated | |
|
|
-9.362 eV/atom | calculated |
|
|
-12.7 kcal/mol=-0.551eV/molicule | reference [20] |
| N
|
8/a |
|
| N
|
4/a |
|
| N |
3/a |
|
| E |
-382.684eV | calculated |
| E |
-389.894eV | calculated |
| E |
-389.896eV | calculated |
| E |
-6.51- |
|
| E |
-7.75- |
|
| E |
-7.752- |
The energy to form a substitutional Zr point defects is approximately 2.8eV and the
energy to form interstitial defects is 1.6eV. The error of energies calculated by
VASP is on the order of
. Ignoring the possible error introduced by
the assumptions, one can approximate the error of these E
energies to be 0.6eV.
These results are of a believable magnitude although one may expect slightly higher
E
values. Maroudas and Brown calculated, via EAM potential, the energy of formation for
silicon vacancy, self-substitution, and self-interstitial
defects to be 2.66eV,
3.09eV, and 4.84eV
respectively. [21] Within the present context there is insufficient information to
explain why the calculated energy of formation for Zr substitutional defects is lower than
Maroudas's energy of formation for vacancies. A more detailed investigation should
yield clues to determining if there is a failure in one of the assumptions from
section 3 or
if this discrepancy in results is indicative of the short comings of EAM methods.
From the results above the equilibrium concentrations of Zr point defects are plotted in
figures 2. From the Arrhenius plot, it is apparent that in the Zr rich
limit (
) the concentration of defects is slightly higher.
At low temperatures the number of interstitial defects dominates the overall number of Zr
defects, but this difference in concentration decreases with increasing temperature. A cross-over
in concentration occurs at around 5000K, a temperature much higher than the melting point
of silicon. It is therefore expected that for all temperatures the concentration of Zr
interstitials will be greater than that of substitutional Zr.
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