University of Houston • University of Houston-Clear Lake • ISSO Annual Report Y2006 • 70
Investigation of III-Nitride Materials for Space-based Solar Cells
ABSTRACT—This project is investigating the suitability of the material InGaN as a candidate for photovoltaic space power generation. The effect of growth parameters on the properties of the films is under study.
The InGaN material system has the capability of covering almost all of the usable solar spectral range (0.5 - 3.0 eV) employed by solar cells. Based on the film composition, InGaN can cover from 0.70 eV up to 3.4 eV, which would be ideal for high efficiency solar cell applications. Also, it has recently been determined that the Nitride materials can offer exceptional radiation tolerance well beyond what can be achieved with conventional solar cell materials currently flown into space.1 However, InGaN is currently a much less mature technology than other III-V semiconductors used in conventional solar cells.
Goal
The goal of this ongoing project is to determine the feasibility of the InGaN material system for use in high efficiency single and multijunction solar cells. Previously, simulations of single junction InGaN solar cells were undertaken to predict the effect of structural defects on the performance of the devices. Simulations verified that InGaN is theoretically a viable candidate for solar cell applications but that improvement in electrical and structural quality was necessary.
Results
Growth of InxGa1-xN films by MBE under different growth conditions — such as In/Ga ratio, total III/N ratio, and film growth rate — have been performed. To date, we have realized a maximum indium mole fraction of approximately 51 percent based on room temperature and low temperature photoluminescence measurements. Thick InGaN for this project faced several challenges: large difference in volatility (evaporation) for indium compared to gallium, much lower growth temperatures needed for indium incorporation compared to pure GaN, and segregation of the indium during the growth which can cause compositional fluctuations.
Currently, samples in the higher indium mole fraction range exhibit some compositional fluctuations and increased background conductivity, but it is expected that further growth refinements should be able to reduce or eliminate these effects. These refinements include improved deposition parameters and exploration of a flux modulation approach to the InGaN deposition. Modulating the arrival of the metal and nitrogen fluxes to the substrate can improve adatom mobility at the lower growth temperatures and help suppress compositional fluctuations.
References
1J. W. Ager III, J. Wu, K. M. Yu, R. E. Jones, S. X. Li, W. Walukiewicz, E. E. Haller, H. Lu, and W. J. Schaff, "Group III-Nitride Alloys as Photovoltaic Materials," Proc. SPIE 5530 (2004): 308-15.
Institute for Space Systems Operations - Y2006 Annual Report
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