Understanding Time Scales of Ionic and Electronic Phenomena in Perovskite Solar Cells
Juan Bisquert a
a Universitat Jaume I, Institute of Advanced Materials (INAM) - Spain, Avinguda de Vicent Sos Baynat, Castelló de la Plana, Spain
Materials for Sustainable Development Conference (MATSUS)
Proceedings of nanoGe Fall Meeting19 (NFM19)
#PERInt19. Interplay of composition, structure and electronic properties in halide-perovskites
Berlin, Germany, 2019 November 3rd - 8th
Organizers: Mahshid Ahmadi, Efrat Lifshitz, Cristiane Morais Smith, Marcus Scheele, Roel van de Krol, Pablo P. Boix, Erwin Reisner, Stefan Weber, Germà Garcia-Belmonte, Doron Naveh and Maksym Yarema
Keynote, Juan Bisquert, presentation 197
DOI: https://doi.org/10.29363/nanoge.nfm.2019.197
Publication date: 18th July 2019

We suggest a classification of the time scales for ionic/electronic phenomena in the perovskite solar cells, based on the results of analysis of kinetic phenomena using frequency modulated techniques and time transient techniques. First with impedance spectroscopy we provide an interpretation of capacitances as a function of frequency both in dark and under light, and we discuss the meaning of resistances and how they are primarily related to the operation of contacts in many cases. The capacitance reveals a very large charge accumulation at the electron contact, which has a great impact in the cell measurements, both in photovoltage decays, recombination, and hysteresis. We also show the identification of the impedance of ionic diffusion by measuring single crystal samples. The attachment of ions to the electrode surface appears as the major factor responsible for hysteresis in perovskite solar cells. Working in samples with lateral contacts, we can identify the effect of ionic drift on changes of photoluminescence, by the creation of recombination centers in defects of the structure. We also address new methods of characterization of the optical response by means of light modulated spectroscopy. The combination of IMPS and Impedance Spectroscopy is able to provide a detailed picture that explains low frequency characteristics, influencing the fill factor of the solar cell.

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