%0 Conference Proceedings
%T X-ray diffraction study of A- plane non polar InN epilayer grown by MOCVD
%+ Laboratoire Charles Coulomb (L2C)
%A Moret, Matthieu
%A Briot, Olivier
%A Gil, Bernard
%< avec comité de lecture
%Z L2C:15-046
%( Proceedings of SPIE
%B GALLIUM NITRIDE MATERIALS AND DEVICES X
%C San Francisco, United States
%Y Society of Photo-Optical Instrumentation Engineers (SPIE)
%3 Proc. SPIE
%V 9363
%P 936328
%8 2015
%D 2015
%R 10.1117/12.2077513
%K Indium Nitride
%K Non polar
%K X ray diffraction
%K Reciprocal space mapping
%Z Physics [physics]/Condensed Matter [cond-mat]/Materials Science [cond-mat.mtrl-sci]Conference papers
%X Strong polarisation-induced electric fields in C-plane oriented nitrides semiconductor layers reduce the performance of devices. Eliminating the polarization fields can be achieved by growing nitrides along non polar direction. We have grown non polar A-plane oriented InN on R-plane (1‾102) nitridated sapphire substrate by MOCVD. We have studied the structural anisotropy observed in these layers by analyzing High Resolution XRay Diffraction rocking curve (RC) experiments as a function of the in-plane beam orientation. A-plane InN epilayer have a unique epitaxial relationship on R-Plane sapphire and show a strong structural anisotropy. Full width at half maximum (FWHM) of the InN(11‾20) XRD RC values are contained between 44 and 81 Arcmin. FWHM is smaller when the diffraction occurs along the [0001] and the largest FWHM values, of the (11‾20) RC, are obtained when the diffraction occurs along the [1‾100] in-plane direction. Atomic Force Microscopy imaging revealed morphologies with well organized crystallites. The grains are structured along a unique crystallographic orientation of InN, leading to larger domains in this direction. This structural anisotropy can be, in first approximation, attributed to the difference in the domain sizes observed. XRD reciprocal space mappings (RSM) were performed in asymmetrical configuration on (13‾40) and (2‾202) diffraction plane. RSM are measured with a beam orientation corresponding to a maximal and a minimal width of the (11‾20) Rocking curves, respectively. A simple theoretical model is exposed to interpret the RSM. We concluded that the dominant contribution to the anisotropy is due to the scattering coherence length anisotropy present in our samples. © (2015) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE)
%G English
%L hal-01134316
%U https://hal.science/hal-01134316
%~ CNRS
%~ L2C
%~ MIPS
%~ UNIV-MONTPELLIER
%~ UM-2015-2021