Abstract
The observed junction between α-CuInSe2 and the In-rich compositions in the β-phase domain (e.g. CuIn3Se5) appears to play an important role in the photovoltaic process. There remain, however, inconsistencies and uncertainties about the boundary and structure of this phase. In general the structure of this phase belongs to defect tetrahedral family of structures, which can be described as normal tetrahedral structures with a certain fixed number of unoccupied structure sites. In this work, the local structures of various (Cu2Se)x(In2Se3)1-x semiconductor alloys in the β-phase domain were studied by Extended X-ray Absorption Fine Structure (EXAFS) and the results were compared to those for the α-CuInSe2 phase. The long-range order of these compositions was studied by X-Ray powder Diffraction (XRD) and electron diffraction. It was found the local structures of these compounds are well defined. These compounds, however, could not be well described by any long-range order structure model, especially the selenium position. First-principles band structure calculations were performed to assist in assigning crystal structures to CuInSe2, CuIn3Se5 and CuIn5Se8. The calculations indicated that the local environments of these compounds are well defined. Their long-range order might depend sensitively on growth history and the configurational entropies as suggested by the similar formation energies of several possible crystal structures for CuIn3Se5 and CuIn5Se8.
| Original language | English |
|---|---|
| Pages (from-to) | H431-H436 |
| Journal | Materials Research Society Symposium - Proceedings |
| Volume | 668 |
| DOIs | |
| State | Published - 2001 |
| Event | II - VI Compound Semiconductor Photovoltaic Materials - San Francisco, CA, United States Duration: Apr 16 2001 → Apr 20 2001 |
Funding
The authors wish to thank A. Zunger at NREL for his helpful discussions, N. Leyarovska at the APS, ANL for her assistance with the EXAFS experiments, and R.N Bhattacharya at NREL for the ICP measurements. The work at UF was supported by the DOE/NREL Thin Film PV Partnership Program under subcontract XAF-5-14142-10. Use of the APS was supported by the U. S. DOE, BES, Office of Science, under Contract No. W-31-109-Eng-38. The U. S. DOE under contract No. DE-AC36-98-GO10337 supported the work at NREL. The use of diffraction user facility at HTML, ORNL, is sponsored by the U.S. Dept. of Energy under contract DE-AC05-00OR22725.
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