Abstract
II-IV-V2 materials, ternary analogs to III-V materials, are emerging for their potential applications in devices such as LEDs and solar cells. Controlling cation ordering in II-IV-V2 materials offers the potential to tune properties at nearly fixed compositions and lattice parameters. While tuning properties at a fixed lattice constant through ordering has the potential to be a powerful tool used in device fabrication, cation ordering also creates challenges with characterization and quantification of ordering. In this work, we investigate two different methods to quantify cation ordering in ZnGeP2 thin films: a stretching parameter calculated from lattice constants, and an order parameter determined from the cation site occupancies (S). We use high resolution X-ray diffraction (HRXRD) to determine and resonant energy X-ray diffraction (REXD) to extract S. REXD is critical to distinguish between elements with similar Z-number (e.g. Zn and Ge). We found that samples with a corresponding to the ordered chalcopyrite structure had only partially ordered S values. The optical absorption onset for these films occurred at lower energy than expected for fully ordered ZnGeP2, indicating that S is a more accurate descriptor of cation order than the stretching parameter. Since disorder is complex and can occur on many length scales, metrics for quantifying disorder should be chosen that most accurately reflect the physical properties of interest.
Original language | English |
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Pages (from-to) | 4350-4356 |
Number of pages | 7 |
Journal | Journal of Materials Chemistry C |
Volume | 8 |
Issue number | 13 |
DOIs | |
State | Published - Apr 7 2020 |
Externally published | Yes |
Funding
This work was authored in part by Alliance for Sustainable Energy, LLC, the manager and operator of the National Renewable Energy Laboratory for the U.S. Department of Energy (DOE) under Contract No. DE-AC36-08GO28308. Primary support for this work was provided by the U.S. Department of Energy, Office of Science, Basic Energy Sciences, Materials Sciences and Engineering Division. R. R. S. acknowledges support from the National Science Foundation Graduate Research Fellowship under Grant No. 1646713. B. L.-W. acknowledges support from the National Science Foundation Graduate Research Fellowship under Grant No. DGE-114747. B. L.-W., M. F. T., and E. S. T. acknowledge support from the National Science Foundation, DMREF No. 1729594. Use of the Stanford Synchrotron Radiation Lightsource, SLAC National Accelerator Laboratory, is supported by the DOE Office of Science (SC), Basic Energy Sciences (BES) under Contract No. DE-AC02-76SF00515. The authors are also grateful to Jacob Cordell and Dr Stephan Lany for many helpful discussions.
Funders | Funder number |
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DMREF | |
DOE Office of Science | DE-AC02-76SF00515 |
National Science Foundation | 1646713, DGE-114747 |
U.S. Department of Energy | DE-AC36-08GO28308 |
Directorate for Mathematical and Physical Sciences | 1729594 |
Office of Science | |
Basic Energy Sciences | |
National Renewable Energy Laboratory | |
Division of Materials Sciences and Engineering |