Earth-abundant, environment-benign, cost-effective, and reliable renewable energy sources are urgently needed to meet the soaring global energy demands. Currently, solar cells based on chalcopyrite Cu(In,Ga)Se 2 (CIGSe) absorbers have yielded the highest power conversion efficiency (η) among all-inorganic thin-film technologies. [1] However, due to the scarcity of In and Ga in the Earth's crust, it would be difficult to satisfy the demands for terawatt (TW)-scale deployment using CIGSe-based cells. Kesterite Cu 2 ZnSnS 4 (CZTS), a derivative of CIGSe, is a promising candidate that satisfies all the aforementioned criteria for next-generation large-scale photovoltaic applications. However, the lower η of CZTS solar cells relative to CIGSe counterparts is still a major challenge for the development of kesterite solar cells. [2][3][4][5][6][7] The main bottleneck is the open-circuit voltage (V OC ) deficit (defined as E g /q À V OC , where E g and q respectively represent bandgap energy and the unit charge), primarily induced by large Shockley-Read-Hall (SRH) recombination at the CZTS/CdS heterointerface [8][9][10][11] and