April 22 - 26, 2024
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EN10.19.03

Local Background Hole Density Drives Non-Radiative Recombination in Tin Halide Perovskites

When and Where

Apr 26, 2024
11:00am - 11:15am
Room 334, Level 3, Summit

Presenter(s)

Co-Author(s)

Robert Westbrook1,Margherita Taddei1,Rajiv Giridharagopal1,Meihuizi Jiang2,Shaun Gallagher1,Kathryn Guye1,3,Aaron Warga1,Saif Haque2,David Ginger1,3

University of Washington1,Imperial College London2,Pacific Northwest National Laboratory3

Abstract

Robert Westbrook1,Margherita Taddei1,Rajiv Giridharagopal1,Meihuizi Jiang2,Shaun Gallagher1,Kathryn Guye1,3,Aaron Warga1,Saif Haque2,David Ginger1,3

University of Washington1,Imperial College London2,Pacific Northwest National Laboratory3
Tin halide perovskites, with the general formula ABX3 [A = Formamidinium (FA), B = Sn, X = Br, I], offer a narrower bandgap (~1.3 eV) than their lead counterparts, making them suitable candidates for the light-absorbing semiconductor in single-junction photovoltaic devices. Moreover, this attribute makes tin halide perovskites integral to all-perovskite tandems, with the best-performing cells incorporating a 50-50 Sn-Pb composition in the low bandgap component. Nevertheless, record-breaking pure-Sn devices still exhibit severe losses in both open-circuit voltage (VOC) and short-circuit current (JSC), keeping power conversion efficiencies well below theoretical limits.
Non-radiative voltage loss is directly linked to decreases in the photoluminescence quantum yield (PLQY), and thus the prevalence of non-radiative recombination.[1] This picture is complicated in Sn perovskites given that the presence of Sn4+ impurities in the precursor solution leads to both the introduction of background hole dopants (serving to increase the PLQY) and non-radiative recombination centers (serving to decrease the PLQY). [2]
We use the observation of pseudo-first order photoluminescence (PL) decay kinetics in Sn perovskite films to establish a method for characterizing the hole dopant level and non-radiative recombination rate constant with combined time-correlated single photon counting (TCSPC) and photoluminescence quantum yield (PLQY) measurements. We find that untreated FASnI3 films exhibit large hole doping concentrations of p0 > 8.8 x 1018 cm-3, which is reduced to p0 ~ 1016 cm-3 after precursor sublimation and SnF2 treatments. While it is well known that the radiative recombination rates are increased with p0, we reveal that the non-radiative rate is also increased. Employing hyperspectral photoluminescence microscopy, we find that microscale p-type regions in untreated FASnI3 films are centers for non-radiative recombination, which are diminished in films with p0 ~ 1016 cm-3. We find significant PL heterogeneity even in FASnI3 films with moderate dopant levels, suggesting that new strategies to eliminate deleterious defects in FASnI3 should be developed. [3]

[1] Y. Shi et al, (3-Aminopropyl)Trimethoxysilane Surface Passivation Improves Perovskite Solar Cell Performance by Reducing Surface Recombination Velocity. ACS Energy Lett 2022, 7 (11), 4081–4088. https://doi.org/10.1021/acsenergylett.2c01766.
[2] D. Meggiolaro et al, Tin versus Lead Redox Chemistry Modulates Charge Trapping and Self-Doping in Tin/Lead Iodide Perovskites. Journal of Physical Chemistry Letters 2020, 11 (9), 3546–3556. https://doi.org/10.1021/acs.jpclett.0c00725.
[3] Westbrook et al, Local Background Hole Density Drives Non-Radiative Recombination in Tin Halide Perovskites, Under Review

Keywords

microstructure

Symposium Organizers

Ivan Mora-Sero, Universitat Jaume I
Michael Saliba, University of Stuttgart
Carolin Sutter-Fella, Lawrence Berkeley National Laboratory
Yuanyuan Zhou, Hong Kong University of Science and Technology

Symposium Support

Silver
Journal of Energy Chemistry

Session Chairs

Sascha Feldmann
Raphael Moral

In this Session