Proceedings of nanoGe Fall Meeting 2021 (NFM21)
DOI: https://doi.org/10.29363/nanoge.nfm.2021.111
Publication date: 23rd September 2021
Lead-halide perovskite thin films have successfully been incorporated as light-absorbing and -emitting layers in a wide range of optoelectronic applications.[1,2] Cs2AgBiBr6 (CABB) has been proposed as a promising non-toxic alternative to lead-based perovskites. However, the indirect bandgap and low charge carrier collection efficiencies remain an obstacle for the incorporation of CABB in optoelectronic applications.[3] The limited charge carrier extraction has been ascribed to the high trap density and strong electron-phonon coupling, compared to its lead-containing analogues, resulting in fast charge carrier localization and low charge carrier mobilities. On the other hand, transient absorption experiments show a long-lived charge carrier lifetime ranging over several microseconds.[4] Moreover, at elevated temperatures mobile carriers are observed for microseconds after photoexcitation, highlighting CABB as a potential alternative for lead-halide analogues.[5]
To study the (free) charge-carrier dynamics we have performed transient absorption (TA) spectroscopy and time-resolved microwave conductivity (TRMC) experiments on CABB thin films on nanosecond to microsecond timescales. TA spectroscopy revealed that the charge carrier density decays on a 40-nanosecond timescale but a fraction of the photogenerated holes near the valence band maximum have a lifetime ranging over several microseconds. TRMC measurements showed that these long-lived carriers are, however, not mobile. Comparison of the TRMC and TA traces shows that the conductivity loss is the result of a combined effect of charge carrier loss and localization. Finally, we estimate that the charge carrier diffusion length is ca. 100 nm. This is of the same order of magnitude as the grain size, suggesting that grain boundaries are an important contributor to charge-carrier loss.
Huygen Jöbsis and Eline Hutter acknowledge funding from the Dutch Research Council (NWO) under the grant number VI.Veni.192.034. Huygen Jöbsis and Eline Hutter are further supported by the Advanced Research Center Chemical Building Blocks Consortium (ARC CBBC). Valentina Caselli and Tom Savenije acknowledge funding from the Dutch Research Council (NWO), grant number 739.017.004. Sven Askes acknowledges funding from the Dutch Research Council (NWO), grant number VI.Veni.192.062.