TY - JOUR A1 - Uchida, Ryusuke A1 - Binet, Silvia A1 - Arora, Neha A1 - Jacopin, Gwenole A1 - Alotaibi, Mohammad Hayal A1 - Taubert, Andreas A1 - Zakeeruddin, Shaik Mohammed A1 - Dar, M. Ibrahim A1 - Graetzel, Michael T1 - Insights about the Absence of Rb Cation from the 3D Perovskite Lattice BT - Effect on the Structural, Morphological, and Photophysical Properties and Photovoltaic Performance JF - Small N2 - Efficiencies >20% are obtained from the perovskite solar cells (PSCs) employing Cs+ and Rb+ based perovskite compositions; therefore, it is important to understand the effect of these inorganic cations specifically Rb+ on the properties of perovskite structures. Here the influence of Cs+ and Rb+ is elucidated on the structural, morphological, and photophysical properties of perovskite structures and the photovoltaic performances of resulting PSCs. Structural, photoluminescence (PL), and external quantum efficiency studies establish the incorporation of Cs+ (x < 10%) but amply rule out the possibility of Rb-incorporation into the MAPbI(3) (MA = CH3NH3+) lattice. Moreover, morphological studies and time-resolved PL show that both Cs+ and Rb+ detrimentally affect the surface coverage of MAPbI(3) layers and charge-carrier dynamics, respectively, by influencing nucleation density and by inducing nonradiative recombination. In addition, differential scanning calorimetry shows that the transition from orthorhombic to tetragonal phase occurring around 160 K requires more thermal energy for the Cs-containing MAPbI(3) systems compared to the pristine MAPbI(3). Investigation including mixed halide (I/Br) and mixed cation A-cation based compositions further confirms the absence of Rb+ from the 3D-perovskite lattice. The fundamental insights gained through this work will be of great significance to further understand highly promising perovskite compositions. KW - cation miscibility KW - cesium cation KW - perovskite solar cells KW - rubidium cation KW - X-ray diffraction Y1 - 2018 U6 - https://doi.org/10.1002/smll.201802033 SN - 1613-6810 SN - 1613-6829 VL - 14 IS - 36 PB - Wiley-VCH CY - Weinheim ER - TY - JOUR A1 - Wolff, Christian Michael A1 - Caprioglio, Pietro A1 - Stolterfoht, Martin A1 - Neher, Dieter T1 - Nonradiative Recombination in Perovskite Solar Cells BT - the Role of Interfaces JF - Advanced materials N2 - Perovskite solar cells combine high carrier mobilities with long carrier lifetimes and high radiative efficiencies. Despite this, full devices suffer from significant nonradiative recombination losses, limiting their V-OC to values well below the Shockley-Queisser limit. Here, recent advances in understanding nonradiative recombination in perovskite solar cells from picoseconds to steady state are presented, with an emphasis on the interfaces between the perovskite absorber and the charge transport layers. Quantification of the quasi-Fermi level splitting in perovskite films with and without attached transport layers allows to identify the origin of nonradiative recombination, and to explain the V-OC of operational devices. These measurements prove that in state-of-the-art solar cells, nonradiative recombination at the interfaces between the perovskite and the transport layers is more important than processes in the bulk or at grain boundaries. Optical pump-probe techniques give complementary access to the interfacial recombination pathways and provide quantitative information on transfer rates and recombination velocities. Promising optimization strategies are also highlighted, in particular in view of the role of energy level alignment and the importance of surface passivation. Recent record perovskite solar cells with low nonradiative losses are presented where interfacial recombination is effectively overcome-paving the way to the thermodynamic efficiency limit. KW - interfacial recombination KW - open-circuit voltage KW - perovskite solar cells KW - photoluminescence Y1 - 2019 U6 - https://doi.org/10.1002/adma.201902762 SN - 0935-9648 SN - 1521-4095 VL - 31 IS - 52 PB - Wiley-VCH CY - Weinheim ER -