Abstract
In 2Se 3, Cu 2Se, and CuInSe2 thin films have been successfully fabricated using novel metal organic decomposition (MOD) precursors and atmospheric pressure-based deposition and processing. The phase evolution of the binary (In-Se and Cu-Se) and ternary (Cu-In-Se) MOD precursor films was examined during processing to evaluate the nature of the phase and composition changes. The In-Se binary precursor exhibits two specific phase regimes: (i) a cubic-In xSe y phase at processing temperatures between 300 and 400 °C and (ii) the γ-In 2Se 3 phase for films annealed above 450 °C. Both phases exhibit a composition of 40 at.% indium and 60 at.% selenium. The binary Cu-Se precursor films show more diverse phase behavior, and within a narrow temperature processing range a number of Cu-Se phases, including CuSe 2, CuSe, and Cu 2Se, can be produced and stabilized. The ternary Cu-In-Se precursor can be used to produce relatively dense CuInSe 2 films at temperatures between 300 and 500 °C. Layering the binary precursors together has provided an approach to producing CuInSe 2 thin films; however, the morphology of the layered binary structure exhibits a significant degree of porosity. An alternative method of layering was explored where the Cu-Se binary was layered on top of an existing indium-gallium-selenide layer and processed. This method produced highly dense and large-grained (<3 μm) CuInSe 2 thin films. This method has significant potential as a manufacturable route to CIGS-based solar cells.
Original language | American English |
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Pages (from-to) | 1375-1387 |
Number of pages | 13 |
Journal | Journal of Materials Research |
Volume | 24 |
Issue number | 4 |
DOIs | |
State | Published - Apr 2009 |
NREL Publication Number
- NREL/JA-520-45841
Keywords
- materials science
- photovoltaics
- semiconductors
- solar energy