4.0 Article

Self-Induced Core-Shell InAlN Nanorods: Formation and Stability Unraveled by Ab Initio Simulations

Journal

ACS NANOSCIENCE AU
Volume 3, Issue 1, Pages 84-93

Publisher

AMER CHEMICAL SOC
DOI: 10.1021/acsnanoscienceau.2c00041

Keywords

self-induced InAlN core-shell nanorods; synthetic growth concept; DFT; reactive magnetron sputter epitaxy; precursor species; nucleation and structural evolution of nanostructures; immiscible systems at nanoscale

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Translated: By using the DFT-based synthetic growth concept, this study explores the formation mechanism of self-induced InAlN core-shell nanorods synthesized by reactive magnetron sputter epitaxy. The study evaluates the characteristics of In- and Al-containing precursor species and finds that In-containing precursors are more prone to dissociation and have lower abundance in the growth environment. The study also examines the incorporation of Al- and In-containing precursor species at the growing edge of the nanorods and correlates it with the experimentally obtained core-shell structure. Additionally, the study shows that the cohesive energies and band gaps of the nanorods decrease with increasing In concentration and overall thickness.
By addressing precursor prevalence and energetics using the DFT-based synthetic growth concept (SGC), the formation mechanism of self-induced InAlN core-shell nanorods (NRs) synthesized by reactive magnetron sputter epitaxy (MSE) is explored. The characteristics of In- and Al-containing precursor species are evaluated considering the thermal conditions at a typical NR growth temperature of around 700 degrees C. The cohesive and dissociation energies of In-containing precursors are consistently lower than those of their Alcontaining counterparts, indicating that In-containing precursors are more weakly bonded and more prone to dissociation. Therefore, Incontaining species are expected to exhibit lower abundance in the NR growth environment. At increased growth temperatures, the depletion of In-based precursors is even more pronounced. A distinctive imbalance in the incorporation of Al- and In-containing precursor species (namely, AlN/AlN+, AlN2/AlN2+, Al2N2/Al2N2+, and Al-2/Al-2(+) vs InN/InN+, InN2/InN2+, In2N2/In2N2+, and In-2/In-2(+)) is found at the growing edge of the NR side surfaces, which correlates well with the experimentally obtained core-shell structure as well as with the distinctive In-rich core and vice versa for the Al-rich shell. The performed modeling indicates that the formation of the core-shell structure is substantially driven by the precursors' abundance and their preferential bonding onto the growing edge of the nanoclusters/islands initiated by phase separation from the beginning of the NR growth. The cohesive energies and the band gaps of the NRs show decreasing trends with an increment in the In concentration of the NRs' core and with an increment in the overall thickness (diameter) of the NRs. These results reveal the energy and electronic reasons behind the limited growth (up to similar to 25% of In atoms of all metal atoms, i.e., InxAl1-xN, x similar to 0.25) in the NR core and may be qualitatively perceived as a limiting factor for the thickness of the grown NRs (typically <50 nm).

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