Robust Molecular Dipole‐Enabled Defect Passivation and Control of Energy‐Level Alignment for High‐Efficiency Perovskite Solar Cells
Affiliation
Department of Chemistry and Biochemistry, The University of ArizonaIssue Date
2021-06-30Keywords
chlorosilane moleculesdefect passivation
dipole moment
interface energy level alignment
perovskite solar cells
Metadata
Show full item recordPublisher
WileyCitation
Wang, B., Li, H., Dai, Q., Zhang, M., Zou, Z., Brédas, J.-L., & Lin, Z. (2021). Robust Molecular Dipole-Enabled Defect Passivation and Control of Energy-Level Alignment for High-Efficiency Perovskite Solar Cells. Angewandte Chemie - International Edition.Rights
© 2021 Wiley-VCH GmbH.Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.Abstract
The ability to passivate defects and modulate the interface energy-level alignment (IEA) is key to boost the performance of perovskite solar cells (PSCs). Herein, we report a robust route that simultaneously allows defect passivation and reduced energy difference between perovskite and hole transport layer (HTL) via the judicious placement of polar chlorine-terminated silane molecules at the interface. Density functional theory (DFT) points to effective passivation of the halide vacancies on perovskite surface by the silane chlorine atoms. An integrated experimental and DFT study demonstrates that the dipole layer formed by the silane molecules decreases the perovskite work function, imparting an Ohmic character to the perovskite/HTL contact. The corresponding PSCs manifest a nearly 20 % increase in power conversion efficiency over pristine devices and a markedly enhanced device stability. As such, the use of polar molecules to passivate defects and tailor the IEA in PSCs presents a promising platform to advance the performance of PSCs. © 2021 Wiley-VCH GmbHNote
12 month embargo; first published: 09 June 2021ISSN
1433-7851EISSN
1521-3773Version
Final accepted manuscriptSponsors
National Science Foundationae974a485f413a2113503eed53cd6c53
10.1002/anie.202105512