Low Frequency Carrier Kinetics in Perovskite Solar Cells

TL;DR

This study uses low-frequency noise and impedance spectroscopy to investigate carrier kinetics in perovskite solar cells, revealing how different materials affect device performance and stability.

Contribution

It introduces correlated low-frequency noise and impedance spectroscopy as a novel method to analyze carrier kinetics in operating perovskite solar cells.

Findings

PTAA cells show a Lorentzian feature at 200 Hz in noise measurements.

Spiro-OMeTAD cells exhibit significantly lower noise amplitude and cyclostationary processes.

Noise amplitude correlates with power conversion efficiency and fill factor.

Abstract

Hybrid organic-inorganic halide perovskite solar cells have emerged as leading candidates for third-generation photovoltaic technology. Despite the rapid improvement in power conversion efficiency (PCE) for perovskite solar cells in recent years, the low-frequency carrier kinetics that underlie practical roadblocks such as hysteresis and degradation remain relatively poorly understood. In an effort to bridge this knowledge gap, we perform here correlated low-frequency noise (LFN) and impedance spectroscopy (IS) characterization that elucidates carrier kinetics in operating perovskite solar cells. Specifically, we focus on planar cell geometries with a SnO2 electron transport layer and two different hole transport layers, namely, poly(triarylamine) (PTAA) and Spiro-OMeTAD. PTAA and Sprio-OMeTAD cells with moderate PCEs of 5 to 12 percent possess a Lorentzian feature at 200 Hz in LFN measurements that corresponds to a crossover from electrode to dielectric polarization. In comparison, Spiro-OMeTAD cells with high PCEs (15 percent) show four orders of magnitude lower LFN amplitude and are accompanied by a cyclostationary process. Through a systematic study of more than a dozen solar cells, we establish a correlation with noise amplitude, power conversion efficiency, and fill factor. Overall, this work establishes correlated LFN and IS as an effective methodology for quantifying low frequency carrier kinetics in perovskite solar cells, thereby providing new physical insights that can rationally guide ongoing efforts to improve device performance, reproducibility, and stability.