2010
DOI: 10.1016/j.jcrysgro.2009.10.066
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InN layers grown by MOCVD on substrates

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Cited by 10 publications
(7 citation statements)
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References 23 publications
(25 reference statements)
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“…2. A flake-like growth mode is found in the w-InN films, which is similar to that of w-InN films on (111) STO substrates [16]. However, it turns into a long strip shape in the same direction in zb-InN films, in accordance with the rather different lattice mismatch in the two vertical directions of [100] STO and [011] STO .…”
Section: Resultssupporting
confidence: 65%
“…2. A flake-like growth mode is found in the w-InN films, which is similar to that of w-InN films on (111) STO substrates [16]. However, it turns into a long strip shape in the same direction in zb-InN films, in accordance with the rather different lattice mismatch in the two vertical directions of [100] STO and [011] STO .…”
Section: Resultssupporting
confidence: 65%
“…InN is a kind of piezoelectric crystal, so the strain existing in the InN overlayer of the heterojunction will induce piezoelectric field and affect the results. According to the previous reports, we know the lattice mismatch between InN and STO is larger than 9.8% inferred from the Φ scanning patterns of InN film grown on STO [ 10 ].The majority of the strain relaxes within the first few monolayers in the InN film, so the InN layer can be approximately treated as completely relaxed and this approximation should not introduce much error in our result. In addition, InN always exhibits obvious electron accumulation at its surface and causes the band bending downward (approximately 0.6 eV) near the surface [ 23 - 25 ].…”
Section: Resultsmentioning
confidence: 99%
“…InN films were grown on STO substrate with the trimethylindium and ammonia as the precursors and nitrogen as the carrier gas. Further details of the growth parameters are reported elsewhere [ 10 ]. XPS measurements were performed on a VG MKII XPS instrument with Al Kα ( hv = 1486.6eV) as the x-ray radiation source, which had been calibrated on work function and Fermi energy level ( E F ).…”
Section: Methodsmentioning
confidence: 99%
“…The thick and thin heterostructures of InN/BTO were deposited by metal-organic chemical vapor deposition (MOCVD) at 520°C. More growth condition details of the InN layer can be found in our previous report [9]. XPSs were performed on a PHI Quantera SXM instrument with Al K α ( hν = 1486.6 eV) as the X-ray radiation source, which had been carefully calibrated on work function and Fermi energy level ( E F ).…”
Section: Methodsmentioning
confidence: 99%