A study on the formation of thin-film CZTS solar cells via the aprotic molecular ink approach

Research output: Contribution to conferencePosterResearchpeer-review

52 Downloads (Pure)

Abstract

The DMSO aprotic molecular ink route has recently proven a competitive approach for synthesis of the sulfo-selenide Cu2ZnSn(S,Se)4 with power conversion efficiencies exceeding 10% [Xin2014, Haass2015, Clark2017]. Meanwhile, limited effort has been devoted to synthesis of the pure-sulfide Cu2ZnSnS4 (CZTS) from the solvent DMSO, even though the sulfide kesterite and its alloys have more favorable band gaps for advanced tandem concepts. In this work, CZTS solar cells with an efficiency of 4.65% were synthesized under ambient conditions. This was achieved without an anti-reflective coating, any cation incorporation, or regulated alkali doping.
We map out the process from ink to film to understand the mechanism of formation. Several things happen from once you mix your salts until the final film has formed. We review processes such as complex formation, the thermal behavior of the ink, and how the film dries and crystallizes.
For formulating the ink, we investigate the optimal sulfur-to-metal ratio in the ink by Raman spectroscopy. Furthermore, ICP-OES is used to evaluate the reproducibility of the composition of the ink, and whether it is affected by filtering. The thermal behavior of the ink is analyzed and we find that more than 90% of the mixture has evaporated at 250oC. Furthermore, mass spectrometry reveals that most of the complexes have thermally decomposed at this temperature, while chlorine and sulfoxide species are continually released until 500oC.
For thin-film deposition, spin-coating is used, where a standard deposition routine includes repeated steps of (1) spin-coating, (2) pre-annealing on a hot plate, and (3) cooling. Here, we study different thermal exposure during pre-annealing ranging from 10 s at 250oC to 30 s at 450oC. The investigation resulted in the following observations: Optical microscopy revealed a so-called “worm-like pattern” in the spin-coating films at low thermal exposure, which causes micro-inhomogeneities in film morphology. This pattern is seen to disappear at higher temperatures. Nonetheless, the best devices were fabricated at a lower thermal exposure, because the short-circuit current (JSC) drops as temperature is increased. The reason could be found in the film structure: A lower thermal exposure during pre-annealing results in larger grains and a thicker MoS2 layer at the CZTS/Mo interface. On the other hand, devices completed at higher pre-annealing temperatures display incomplete sulfurizations with smaller grains and the existence of a fine-grain layer at the back interface.
Original languageEnglish
Publication date2020
Publication statusPublished - 2020
Event11th European Kesterite+ online workshop - Virtual event
Duration: 26 Nov 202027 Nov 2020
https://www.kesteriteworkshop2020.com/home

Conference

Conference11th European Kesterite+ online workshop
LocationVirtual event
Period26/11/202027/11/2020
Internet address

Fingerprint

Dive into the research topics of 'A study on the formation of thin-film CZTS solar cells via the aprotic molecular ink approach'. Together they form a unique fingerprint.

Cite this