AVS 60th International Symposium and Exhibition | |
Thin Film | Friday Sessions |
Session TF+EM+NS+SS-FrM |
Session: | Thin Film: Growth and Characterization III |
Presenter: | M. Wei, University of Central Florida |
Authors: | M. Wei, University of Central Florida R.C. Boutwell, University of Central Florida N. Faleev, Arizona State University A. Osinsky, Agnitron Technology Inc. R. Miller, Agnitron Technology Inc. W.V. Schoenfeld, University of Central Florida |
Correspondent: | Click to Email |
Wide band gap semiconductors such as MgxZn1-xO represent an excellent choice for making optical photodetectors and emitters operating in the UV spectral region. High crystal and optical quality MgxZn1-xO thin films were grown epitaxially on c-plane sapphire substrates by plasma-assisted Molecular Beam Epitaxy. ZnO thin films with high crystalline quality, low defect and dislocation densities, and sub-nanometer surface roughness were achieved by applying a low temperature nucleation layer. The critical growth conditions were discussed to obtain a high quality film: the sequence of Zn and O sources for initial growth of nucleation layer, growth temperatures for both ZnO nucleation and growth layers, and Zn/O ratio. Resultant epitaxial ZnO films demonstrated a root-mean-square surface roughness of 0.373nm for 1μm × 1μm atomic force microscope images with clear hexagonal shaped terrace steps. The x-ray diffraction FWHM for (0002) peak was measured to be 13 arc sec for ZnO. By tuning Mg/Zn flux ratio, wurtzite MgxZn1-xO thin films with Mg composition as high as x=0.46 were obtained without phase segregation. The steep optical absorption edges were shown with a cut-off wavelength as short as 278nm, indicating of suitability of such material for solar blind photo detectors. Consequently, Metal-Semiconductor-Metal photoconductive and Schottky barrier devices with interdigital electrode geometry and active surface area of 1 mm2 were fabricated and characterized. Photoconductor based on Mg0.46Zn0.54O showed ~102 A/W peak responsivity at wavelength of ~260nm. The spectral cutoff of the devices was close to 315nm with more than two orders of magnitude visible rejection ratio (R260nm/R400nm) these devices good candidates for solar blind applications.