Competition between Transport and Recombination in Dye Solar Cells at Low Light Intensity

• Published in: Solar RRL 2024-05, Vol.8 (10), p.n/a
• Main Authors: Sánchez‐Fernández, Patricia, Aranda, Clara A., Escalante, Renán, Riquelme, Antonio J., Demadrille, Renaud, Pistor, Paul, Oskam, Gerko, Anta, Juan A.
• Format: Article
• Language: English
• Subjects: Chemical Sciences; dye‐sensitized solar cells; electron transport; Engineering Sciences; impedance spectroscopy; indoor photovoltaics
• ISSN: 2367-198X; 2367-198X
• DOI: 10.1002/solr.202400149

The efficiency of electron collection in a dye‐sensitized solar cell (DSC) is determined by a delicate balance between electronic transport and recombination losses caused by electron transfer to dye cations and electron acceptors. While state‐of‐the‐art DSCs have demonstrated quantitative electron collection under standard 1 sun conditions, the nonlinear nature of the trapping/detrapping dynamics in the photoanode with respect to the stored electronic charge can result in suboptimal performance under the low illumination intensity conditions commonly found indoors. Herein, the key factors influencing electron collection in relation to light intensity using impedance spectroscopy and numerical analysis are thoroughly examined. Impedance analysis reveals that the electron diffusion length tends to decrease as the quasi‐Fermi level is lowered, approaching the critical limit (Ln/d ≈ 1) at intensities characteristic of indoor illumination. A range of tert‐butyl pyridine concentrations and different thermal and chemical treatments of the TiO2 are tested, showing that this low intensity limitation is inherent to the multiple‐trapping mechanism that governs the functioning of a DSC. It is concluded that relatively high ideality factors, nonoptimal electrolyte compositions, or small variations in the quality of the TiO2 layer can result in electron collection limitations that are not apparent under 1 sun but become noticeable at low light intensities. Dye solar cells at low light intensities can have electron collection issues that do now show up at standard 1 sun conditions: “For we do not know what beasts the night dreams when its hours grow too long for even God to be awake”—Hildred Castaigne.