In Situ Mapping of the Molecular Arrangement of Amphiphilic Dye Molecules at the TiO 2 Surface of Dye-Sensitized Solar Cells

Kislon Voïtchovsky, Negar Ashari-Astani, Ivano Tavernelli, Nicolas Tétreault, Ursula Rothlisberger, Francesco Stellacci, Michael Grätzel, Hauke A. Harms

Research output: Contribution to journalArticlepeer-review

30 Scopus citations

Abstract

© 2015 American Chemical Society. Amphiphilic sensitizers are central to the function of dye-sensitized solar cells. It is known that the cell's performance depends on the molecular arrangement and the density of the dye on the semiconductor surface, but a molecular-level picture of the cell-electrolyte interface is still lacking. Here, we present subnanometer in situ atomic force microscopy images of the Z907 dye at the surface of TiO2 in a relevant liquid. Our results reveal changes in the conformation and the lateral arrangement of the dye molecules, depending on their average packing density on the surface. Complementary quantitative measurements on the ensemble of the film are obtained by the quartz-crystal microbalance with dissipation technique. An atomistic picture of the dye coverage-dependent packing, the effectiveness of the hydrophobic alkyl chains as blocking layer, and the solvent accessibility is obtained from molecular dynamics simulations. (Figure Presented).
Original languageEnglish (US)
Pages (from-to)10834-10842
Number of pages9
JournalACS Applied Materials & Interfaces
Volume7
Issue number20
DOIs
StatePublished - May 15 2015
Externally publishedYes

Bibliographical note

KAUST Repository Item: Exported on 2020-10-01
Acknowledged KAUST grant number(s): KUS-C1-015-21
Acknowledgements: K.V. acknowledges funding from the Swiss National Science Foundation through the Ambizione Fellowship (PZ00P2_136941). U.R. acknowledges funding from the Swiss National Science Foundation via individual grant No. 200020-146645, the NCCRs MUST and MARVEL, and support from the Swiss National Computing Center (CSCS) and the CADMOS project for computing resources. M.G. thanks the European Research Council (ERC) for supporting part of this work under the advanced research grant (no. 247404) MESOLIGHT. H.A.H. acknowledges funding from the Swiss National Science Foundation (SNF). M.G. and N.T. acknowledge funding from the King Abdullah University of Science and Technology (KAUST, Award no. KUS-C1-015-21).
This publication acknowledges KAUST support, but has no KAUST affiliated authors.

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