Proceedings of MATSUS23 & Sustainable Technology Forum València (STECH23) (MATSUS23)
DOI: https://doi.org/10.29363/nanoge.matsus.2023.179
Publication date: 22nd December 2022
We fabricate and characterize carbon-based lead halide perovskite solar cells composed of a mesoscopic scaffold of metal oxides that is screen printed and infiltrated with a lead halide perovskite precursor solution with a methylammonium cation.(MAPbI3) We characterize the cells over time to investigate degradation pathways and improve fabrication methods. We measure the current produced by the cells under various illumination conditions as a function of applied bias voltage (IV curves) as well as spatially mapping both the structure and the photovoltaic performance of our cells to track and classify defects using both optical micrographs and Light Beam Induced Current (LBIC) imaging. Observations of the spectral response of the cells enables us to determine the External Quantum Efficiency (EQE) of our devices as well.
In an undergraduate laboratory environment we fabricate and characterize Screen-Printed Mesoporous Carbon Perovskite Solar Cells (CPSCs). The fabrication is based on pioneering work by Hongwei Han's research group.[1] We adapt our methods from those developed by Trystan Watson's group [2]. We start with FTO coated glass substrates and laser engrave isolation lines. We spay coat a compact titania layer followed by screen printing a mesoporous layers of titania (for electron transport), zirconia (for a spacer), and Carbon (for hole transport and a back contact). A Methylammoina Lead Iodide (MAPbI) perovskite precursor is then inflitrated into the mesoporous layers crystalizing to form the perovskite semiconductor structure. Silver contact electrodes are added to complete the devices. The fabrication is performed in an ambient environment and no encapsulations are added to the devices. Each substrate has 36 devices each with an active area of 0.49 sq. cm. We have produced over a thousand devices with 4 generations of students in the lab.
We characterize our devices with a wide range of techniques. Current Voltage characteristics are measured for all devices. Hero cells have power conversion efficiencies over 12%. The devices show negligible hysteresis, and are limited in performance by moderate shunt and series resistances. New higher conductivity Carbon and Silver ink formualations have been tested with significantly better conductivities that have improved Fill Factors and reduced series resistance. We observe a variety of spatial defects by both LBIC and optical micrographs in the printing process and do statistical analysis of yields on every run to optimize our initial device performance. We measure EQEs with peaks approaching 80% for freshly made devcies.
We have performed dark storage shelf life measurements over two years. While devices still work after two years in dark storage, the performance decreases and defects clearly evolve as seen in our spatial imaging over time. We also perform light soaking studies of both individual cells and modules of cells in series. We record not only the IV characteristics and the IV curve evolution, but also the changes in EQE and spatial imaging as a function of light soaking under 1 sun conditions with no encapsulation or UV filtering. We will present these data and discuss what this says about the degradation of these CPSCs.
This work was made possible with support from the National Science Foundation using facilities from the NSF MRI program under award number: 1919282. Summer research students were supported with funds from both Pomona College and the Sontag Family through their Physics Summer Undergraduate Research Grant program. Inital work was made possible by support from the Hirsch Family through their Research Initation Grant program. Bryan Hong contributed to the initial light soaking studies. Scientific advice was provided by both the Watson group at SPECIFIC in Swansea and the Lira Cantu group at ICN2 in Barcelona. Technical and administrative support from the staff of the Pomona College Physics & Astronomy Department was crucial to this work.