Defect physics of the kesterite thin-film solar cell absorber Cu 2 ZnSnS4

Shiyou Chen, X. G. Gong, Aron Walsh, Su Huai Wei

Research output: Contribution to journalArticlepeer-review

503 Scopus citations


Cu2 ZnSnS4 is one of the most promising quaternary absorber materials for thin-film solar cells. Examination of the thermodynamic stability of this quaternary compound reveals that the stable chemical potential region for the formation of stoichiometric compound is small. Under these conditions, the dominant defect will be p -type CuZn antisite, which has an acceptor level deeper than the Cu vacancy. The dominant self-compensated defect pair in this quaternary compound is [CuZn- + Zn Cu+]0, which leads to the formation of various polytype structures of Cu2 ZnSnS4. We propose that to maximize the solar cell performance, growth of Cu2 ZnSnS4 under Cu-poor/Zn-rich conditions will be optimal, if the precipitation of ZnS can be avoided by kinetic barriers.

Original languageEnglish
Article number021902
JournalApplied Physics Letters
Issue number2
StatePublished - 2010


Dive into the research topics of 'Defect physics of the kesterite thin-film solar cell absorber Cu 2 ZnSnS4'. Together they form a unique fingerprint.

Cite this