Proceedings of Online Meetup: Origins of Electronic Defects in Halide Perovskites (EDHP)
Publication date: 1st April 2020
Perovskite photovoltaic (PV) cells have demonstrated power conversion efficiencies (PCE) that are close to those of monocrystalline silicon cells; however, in contrast to silicon PV, perovskites are not limited by Auger recombination under 1‐sun illumination. Nevertheless, compared to GaAs and monocrystalline silicon PV, perovskite cells have significantly lower fill factors due to a combination of resistive and non‐radiative recombination losses. This necessitates a deeper understanding of the underlying loss mechanisms and in particular the ideality factor of the cell. By measuring the intensity dependence of the external open‐circuit voltage and the internal quasi‐Fermi level splitting (QFLS), the transport resistance‐free efficiency of the complete cell as well as the efficiency potential of any neat perovskite film with or without attached transport layers are quantified. Moreover, intensity‐dependent QFLS measurements on different perovskite compositions allows for disentangling of the impact of the interfaces and the perovskite surface on the non‐radiative fill factor and open‐circuit voltage loss. It is found that potassium‐passivated triple cation perovskite films stand out by their exceptionally high implied PCEs > 28%, which could be achieved with ideal transport layers. Finally, strategies are presented to reduce both the ideality factor and transport losses to push the efficiency to the thermodynamic limit.
This work was in part funded by HyPerCells (a joint graduate school of the Potsdam University and the Helmholtz‐Zentrum Berlin) and by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation): project number 423749265. S.D.S. acknowledges funding from the Royal Society and Tata Group (UF150033) and the Engineering and Physical Sciences Research Council (EP/R023980/1). M.A.‐J. acknowledges EPSRC, Cambridge Materials Limited and Wolfson College, University of Cambridge for their funding and technical support. M.G., P.C., S.A., and D.N. acknowledge funding from the Helmholtz Association via HI‐SCORE (Helmholtz International Research School). M.G., P.C., and S.A. acknowledge the Federal Ministry of Education and Research (BMBF) for funding of the Young Investigator Group Perovskite Tandem Solar Cells within the program “Materialforschung fuer die Energiewende” (grant no. 03SF0540). The authors thank Nandi Wu, Daniel Walter, and Klaus Weber from the Australian National University for help and fruitful discussions.