Excited-state structure of copper phenanthroline-based photosensitizers

Alexander Guda, Johannes Windisch, Benjamin Probst, Jeroen A. Van Bokhoven, Roger Alberto, Maarten Nachtegaal, Lin X. Chen, Grigory Smolentsev*

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

11 Scopus citations

Abstract

Cu diimine complexes present a noble metal free alternative to classical Ru, Re, Ir and Pt based photosensitizers in solution photochemistry, photoelectrochemical or dye-sensitized solar cells. Optimization of these dyes requires understanding of factors governing the key photochemical properties: excited state lifetime and emission quantum yield. The involvement of exciplex formation in the deactivation of the photoexcited state is a key question. We investigate the excited-state structure of [Cu(dmp)2]+ and [Cu(dsbtmp)2]+ (dmp = 2,9-dimethyl-1,10-phenanthroline, dsbtmp = 2,9-di-sec-butyl-3,4,7,8-tetramethyl-1,10-phenanthroline) using pump-probe X-ray absorption spectroscopy (XAS) and DFT. Features of XAS that distinguish flattened tetrahedral site and 5-coordinated geometry with an additional solvent near Cu(ii) center are identified. Pump-probe XAS demonstrates that for both complexes the excited state is 4-coordinated. For [Cu(dmp)2]+ the exciplex is 0.24 eV higher in energy than the flattened triplet state, therefore it can be involved in deactivation pathways as a non-observable state that forms slower than it decays. For [Cu(dsbtmp)2]+ the excited-state structure is characterized by Cu-N distances of 1.98 and 2.07 Å and minor distortions, leading to a 3 orders of magnitude longer excited-state lifetime.

Original languageEnglish (US)
Pages (from-to)26729-26736
Number of pages8
JournalPhysical Chemistry Chemical Physics
Volume23
Issue number47
DOIs
StatePublished - Dec 21 2021

Funding

We acknowledge the Paul Scherrer Institute, Villigen, Switzerland for the provision of beamtime at the SuperXAS beamline of the SLS. A. G. acknowledges financial support from Russian Foundation for Basic Research, project 18-02-40029. L. X. C. is supported by the U. S. Department of Energy, Office of Science, Office of Basic Energy Sciences, through Argonne National Laboratory under Contract No. DE-AC02-06CH11357. Furthermore, financial support from the University of Zürich, the University Research Priority Program LightChEC and the Swiss National Science Foundation (Grant CRSII2_160801/1) is acknowledged.

ASJC Scopus subject areas

  • General Physics and Astronomy
  • Physical and Theoretical Chemistry

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