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Stability of Si-interstitial defects: from point to extended defects
Extended interstitial defects in materials transition from compact to rodlike shapes as they grow. This study models defect evolution using simulations, aiding in understanding material properties.
Area of Science:
- Materials Science
- Condensed Matter Physics
- Computational Materials Science
Background:
- Extended interstitial defects influence material properties.
- Understanding defect formation and growth is crucial for materials design.
Purpose of the Study:
- To investigate the growth trends of extended interstitial defects.
- To model the shape evolution of these defects based on their size.
Main Methods:
- Utilized extensive tight-binding and ab initio local density approximation simulations.
- Parametrized defect-formation energy and interstitial capture radius anisotropy.
Main Results:
- Observed a transition in stable defect shape from compact to chainlike to rodlike with increasing interstitials.
- The rodlike 311 defect, originating from (011) chains, stabilizes and elongates as it grows.
- Developed accurate defect-formation energy parameters.
Conclusions:
- Macroscopic defect-growth simulations are enabled by accurate defect energy and capture radius parametrization.
- The study provides insights into the fundamental mechanisms governing interstitial defect evolution in materials.
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