Effect of Temperature, Pressure and Precursor flux ratios on InSb Thin film Growth: Morphology and Properties

POSTER

Abstract

We have investigated the growth of InSb thin films on InAs and GaAs substrates by Chemical Beam Epitaxy (CBE). Raman spectroscopy measurements show that the optical properties of the grown layers is not greatly affected even when varying the growth conditions over a wide range (varying the V/III flux ration between 1 and 10, growth temperature between 390-480$^{\circ}$C). The lattice mismatch between the layers and substrates, results in regions of no growth during the deposition of InSb layers. To circumvent this problem, the growth process is preceded by a 10 mins exposure of the substrates to TMIn. This step eliminates the regions of no growth. Our results show that at constant pressure, the growth rate decreases with increasing temperature and with increasing V/III flux ratio. A much slower response was observed for increasing antimony partial pressure. The lattice mismatch between the layer and substrate give rise to stacking fault and twins. A decrease in particle size from 34.89 to 9.95nm was observed for increasing flux ratio and an increase from11.31 to 32.68nm for increasing temperature. Evidence of Raman spectroscopy results confirms the crystalline nature of the deposited films. Details of our results will be presented at the meeting.

Authors

  • Samuel Mensah

    • Max-Planck Institute of Microstructure Physics
  • Alexander Vogel

    • Max-Planck Institute of Microstructure Physics
  • Joerg Wittemann

    • Max-Planck Institute of Microstructure Physics
  • Johannes de Boor

    • Max-Planck Institute of Microstructure Physics
  • Volker Scmhidt

    • Max-Planck Institute of Microstructure Physics