postdeposition alkali treatment to improve heterojunction diode quality in Cu(In,Ga) Se 2 (CIGS) solar cells and chloride treatment to passivate grain boundaries in CdTe solar cells. [1] These solar-cell technologies are already commercialized, with lab-scale photovoltaic efficiencies exceeding 22%. [2] However, kesterite-based solar cells, such as Cu 2 ZnSn(S,Se) 4 , which share many of the same characteristics of CIGS and CdTe, significantly lag behind, with a record power conversion efficiency (PCE) of 12.6%. [3] Although the dominant limiting factors for this low performance are a matter of considerable discussion, [4] the following observations are consistent among kesterite absorbers: i) a low photoluminescence quantum yield (PLQY) and a short chargecarrier lifetime, [5] ii) a high value of Urbach band tail energy (larger than 30 meV for S-rich kesterites) and lack of a steep absorption onset, [6,7] and iii) the presence of secondary phases. [4,6,8,9] The extent to which these factors individually affect the photovoltaic performance is debated, but their ubiquity among kesterite absorbers indicates the presence of a large density of point defects. [10][11][12] Specifically, i) the low PLQY arises from the presence of nonradiative mid-gap
The identification of performance-limiting factors is a crucial step in the development of solar cell technologies. Cu 2 ZnSn(S,Se) 4 -based solar cells have shown promising power conversion efficiencies in recent years, but their performance remains inferior compared to other thin-film solar cells. Moreover, the fundamental material characteristics that contribute to this inferior performance are unclear. In this paper, the performance-limiting role of deep-trap-level-inducing 2Cu Zn +Sn Zn defect clusters is revealed by comparing the defect formation energies and optoelectronic characteristics of Cu 2 ZnSnS 4 and Cu 2 CdSnS 4 . It is shown that these deleterious defect clusters can be suppressed by substituting Zn withCd in a Cu-poor compositional region. The substitution of Zn with Cd also significantly reduces the bandgap fluctuations, despite the similarity in the formation energy of the Cu Zn +Zn Cu and Cu Cd +Cd Cu antisites. Detailed investigation of the Cu 2 CdSnS 4 series with varying Cu/[Cd+Sn] ratios highlights the importance of Cu-poor composition, presumably via the presence of V Cu , in improving the optoelectronic properties of the cation-substituted absorber. Finally, a 7.96% efficient Cu 2 CdSnS 4 solar cell is demonstrated, which shows the highest efficiency among fully cation-substituted absorbers based on Cu 2 ZnSnS 4 .