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Phase stability and structural comparison of phases in the Cu-Zn-Sn-S system using solid-state NMR.

Authors :
Pogue, Elizabeth A.
Sutrisno, Andre
Johnson, Nicole E.
Goetter, Melissa B.
Jiang, Zhelong
Shoemaker, Daniel P.
Rockett, Angus A.
Source :
Solar Energy Materials & Solar Cells. Feb2019, Vol. 190, p37-48. 12p.
Publication Year :
2019

Abstract

Abstract Phases in the Cu-Zn-Sn-S system are of interest to the solar and thermoelectrics communities because all elements are earth-abundant and non-toxic. A better understanding of the structures of these phases and the equilibria between them is necessary to guide device manufacturers. This work reviews all the phases reported in this system and reports which phases form and are stable at 200 °C and 400 °C. In this work, the stable phases in the Cu-Zn-Sn-S system ( Cu 4 Sn 7 S 16 , Cu 4 SnS 4 , Cu 2 ZnSnS 4 , and Cu 2 SnS 3 ) are synthesized and their structures are investigated using solid-state NMR, X-ray diffraction, and Raman spectroscopy. The existing Cu-Sn-S and Cu-Zn-Sn-S phase diagrams are revised based on our synthesis results. Cu 3 SnS 4 and Cu 2 ZnSn 3 S 8 are removed from the quaternary and ternary phase diagrams because we did not observe either phase. Prior reports (in thin films and nanocrystals) of Cu 3 SnS 4 may be related to trace amounts of In or large surface areas. Monoclinic Cu 2 SnS 3 is not stable at 400 °C and, at this temperature, a disordered tetragonal phase is stable. At lower temperatures (room-temperature and 200 °C), this same (disordered) tetragonal phase is stable at compositions that are Cu-rich and Sn-poor from Cu 2 SnS 3 . Cu 4 SnS 6 was added to the phase diagram at 400 °C. Significant differences in reaction rate when forming Cu 4 SnS 4 from either elemental or binary sulfide precursors are noted and explained. The NMR results are generalized to aid in distinguishing octahedral versus tetrahedral Sn4+ coordinations. Graphical abstract fx1 Highlights • Ss-NMR: useful for studying Sn 4 + coordination and Cu-Zn-Sn-S system structures. • Cu-Zn-Sn-S and Cu-Sn-S phase diagrams at room-temperature, 200 °C, and 400 °C. • Cu 3 SnS 4 reports may be due to indium contamination. • Kinetic barriers to Cu 4 SnS 4 from elemental precursors but not binary precursors. • Order-disorder transitions between 200 °C and 400 °C in Cu 2 SnS 3 and Cu 2 ZnSnS 4 . [ABSTRACT FROM AUTHOR]

Details

Language :
English
ISSN :
09270248
Volume :
190
Database :
Academic Search Index
Journal :
Solar Energy Materials & Solar Cells
Publication Type :
Academic Journal
Accession number :
132869159
Full Text :
https://doi.org/10.1016/j.solmat.2018.10.007