Cu2ZnSnSe4 thin films prepared by selenization of one-step electrochemically deposited Cu–Zn–Sn–Se precursors
► Selenization one-step electrochemical deposition Cu–Zn–Sn–Se precursors to fabricate CZTSe thin films for the first time. ► Studied the effect of different rate of each element in electrolyte and the influence of pH. ► Prepared Cu2ZnSnSe4 that is pure and close to stoichiometric. ► Proved the stru...
Saved in:
Published in | Applied surface science Vol. 273; pp. 613 - 616 |
---|---|
Main Authors | , , , , |
Format | Journal Article |
Language | English |
Published |
Amsterdam
Elsevier B.V
15.05.2013
Elsevier |
Subjects | |
Online Access | Get full text |
Cover
Loading…
Summary: | ► Selenization one-step electrochemical deposition Cu–Zn–Sn–Se precursors to fabricate CZTSe thin films for the first time. ► Studied the effect of different rate of each element in electrolyte and the influence of pH. ► Prepared Cu2ZnSnSe4 that is pure and close to stoichiometric. ► Proved the structure of CZTSe is Kesterite-type.
In this research a non-vacuum strategy was reported in facile preparation of kesterite-type Cu2ZnSnSe4 (CZTSe) thin films via selenization of one-step electrochemically prepared Cu–Zn–Sn–Se precursors. The Cu–Zn–Sn–Se precursor films were prepared by electrochemical deposition from electrolytes containing CuSO4, ZnSO4, SnCl4 and H2SeO3, and the substrate is a Mo coated soda-lime glass. The CZTSe thin films were obtained by annealing the electrochemically deposited films in the selenium vapors at the temperature of 550°C. The crystal phases, micro-structures, chemical compositions and optical properties of CZTSe films have been studied by powder X-ray diffraction (XRD), scanning electron microscopy (SEM), inductively coupled plasma optical emission spectrometer (ICP-OES), Raman scattering spectrum, and UV–vis absorption spectroscopic means. The results revealed that the electrolytes with Cu:Zn:Sn:Se molar ratio of 3:70:20:3 yields nearly pure phase of kesterite, and a band gap of 0.94eV was determined by spectroscopic measurements. |
---|---|
Bibliography: | ObjectType-Article-1 SourceType-Scholarly Journals-1 ObjectType-Feature-2 content type line 23 |
ISSN: | 0169-4332 1873-5584 |
DOI: | 10.1016/j.apsusc.2013.02.088 |