The step-behavior of InGaN thin films grown on sapphire substrates by metal
organic vapor phase epitaxy was studied using atomic force microscopy char
acterization. Spiral size and interstep distance decreased when the supersa
turation of the group-III source was increased. Using this dependency and t
he Burton, Cabrera, and Frank model, the step energy was calculated to be 2
.6 J/m(2) for InN in InGaN and 1.5 J/m(2) for GaN. InGaN spiral growth on s
apphire substrates is caused by the specific large step energy of this mate
rial. Therefore, reducing dislocation densities in the epitaxial layers is
most effective for reducing spiral densities. This was confirmed by growing
InGaN on FIELO-GaN substrates, which have a low dislocation density. (C) 2
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