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Conference paper

Bio-inspired co-catalysts bonded to a silicon photocathode for solar hydrogen evolution

From

Department of Physics, Technical University of Denmark1

Surface Physics and Catalysis, Department of Physics, Technical University of Denmark2

Computational Atomic-scale Materials Design, Department of Physics, Technical University of Denmark3

Haldor Topsoe AS4

Department of Micro- and Nanotechnology, Technical University of Denmark5

Center for Individual Nanoparticle Functionality, Centers, Technical University of Denmark6

The production of fuels directly or indirectly from sunlight represents one of the major challenges to the development of a sustainable energy system. Hydrogen is the simplest fuel to produce and while platinum and other noble metals are efficient catalysts for photoelectrochemical hydrogen evolution, earth-abundant alternatives are needed for largescale use.

We show that bio-inspired molecular clusters based on molybdenum sulfides and tungsten sulfides mimic nature's enzymes for hydrogen evolution, molybdenum sulfides evolve hydrogen at a slightly higher overpotential than platinum when deposited on various supports. It will be demonstrated how this overpotential can be eliminated by depositing the same type of hydrogen evolution catalyst on p-type Si which can harvest the red part of the solar spectrum.

Such a system could constitute the cathode part of a tandem dream device where the red part of the spectrum is utilized for hydrogen evolution while the blue part is reserved for the more difficult oxygen evolution. The samples have been illuminated with a simulated red part of the solar spectrum i.e. long wavelength (" > 620 nm) part of simulated AM 1.5G radiation.

The current densities at the reversible potential match the requirement of a photoelectrochemical hydrogen production system with a solar-to-hydrogen efficiency in excess of 10%. The experimental observations are supported by DFT calculations of the Mo3S4 cluster adsorbed on the hydrogen-terminated silicon surface providing insights into the nature of the active site.

Language: English
Publisher: SPIE - International Society for Optical Engineering
Year: 2011
Pages: 81090Q-8
Proceedings: Solar Hydrogen and Nanotechnology VI
ISSN: 1996756x and 0277786x
Types: Conference paper
DOI: 10.1117/12.892994
ORCIDs: Vesborg, Peter Christian Kjærgaard , Seger, Brian , Pedersen, Thomas , Hansen, Ole , Nørskov, Jens Kehlet and Chorkendorff, Ib

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