TY - JOUR
T1 - An operando x-ray absorption spectroscopy study of a NiCu-TiO2 photocatalyst for H2 evolution
AU - Spanu, Davide
AU - Minguzzi, Alessandro
AU - Recchia, Sandro
AU - Shahvardanfard, Fahimeh
AU - Tomanec, Ondrěj
AU - Zboril, Radek
AU - Schmuki, Patrik
AU - Ghigna, Paolo
AU - Altomare, Marco
N1 - Funding Information:
M.A., F.S., and P.S. acknowledge ERC, DFG, and the DFG cluster of excellence EAM for financial support, as well as H. Hildebrand, A. Friedrich, A. Knoop, and U. Marten-Jahns for technical help. M.A. acknowledges the financial support from the Emerging Talents Initiative ETI (ETI2018/2_Tech_11) provided by the FAU Friedrich-Alexander University Erlangen-Nuremberg, Germany. M.A., P.G., and A.M. acknowledge DESY (Hamburg, Germany), a member of the Helmholtz Association HGF, for the provision of experimental facilities. Parts of this research were carried out at DESY-PETRA III (Project I-20190283), and the authors thank Dr. Edmund Welter for technical assistance in using the photon beamline P65. The research leading to this result has been supported also by the project CALIPSOplus under the Grant Agreement 730872 from the EU Framework Programme for Research and Innovation HORIZON 2020. A.M. acknowledges “Piano di Sostegno alla Ricerca, Università degli Studi di Milano”. P.G. acknowledges financial support by MIUR through the grant “PRIN 2017, 2017KKP5ZR, MOSCATo”. D.S. and S.R. gratefully acknowledge financial support from MIUR.
Funding Information:
M.A., F.S., and P.S. acknowledge ERC, DFG, and the DFG cluster of excellence EAM for financial support, as well as H. Hildebrand, A. Friedrich, A. Knoop, and U. Marten-Jahns for technical help. M.A. acknowledges the financial support from the Emerging Talents Initiative ETI (ETI2018/2_Tech_11) provided by the FAU Friedrich-Alexander University Erlangen-Nuremberg, Germany. M.A., P.G., and A.M. acknowledge DESY (Hamburg, Germany), a member of the Helmholtz Association HGF, for the provision of experimental facilities. Parts of this research were carried out at DESY-PETRA III (Project I-20190283), and the authors thank Dr. Edmund Welter for technical assistance in using the photon beamline P65. The research leading to this result has been supported also by the project CALIPSOplus under the Grant Agreement 730872 from the EU Framework Programme for Research and Innovation HORIZON 2020. A.M. acknowledges ?Piano di Sostegno alla Ricerca, Universita degli Studi di Milano?. P.G. acknowledges financial support by MIUR through the grant ?PRIN 2017, 2017KKP5ZR, MOSCATo?. D.S. and S.R. gratefully acknowledge financial support from MIUR.
Publisher Copyright:
© 2020 American Chemical Society.
PY - 2020/8/7
Y1 - 2020/8/7
N2 - Cu- or Ni-decorated semiconductors represent a potential low-cost alternative to noble-metal-modified photocatalysts. Even more effective are bimetallic NiCu nanoparticles, which can provide a remarkable photocatalytic H2 evolution enhancement compared to single-element Cu or Ni systems. The main concern of such alloyed co-catalysts is their activity with respect to alteration of their elemental composition and oxidation state over reaction time. Ex situ characterization techniques provide controversial interpretations of the co-catalytic role of the individual elements. Hypotheses such as the in situ reduction of “native” Ni or Cu species during photocatalysis, the oxidation of metallic Cu or Ni into oxides or hydroxides, or the formation of p-n junctions or core/shell structures have been proposed. Herein, we present an operando X-ray absorption spectroscopy study of a NiCu-TiO2 system under UV light illumination in ethanol-water solutions, i.e., under photocatalytic H2 evolution conditions. The experimental approach allows for monitoring in real time chemical changes that take place in the co-catalyst under intermittent illumination, i.e., under light on-off cycles. We show that while Ni and Cu are partially oxidized in the as-formed NiCu co-catalyst (air-formed surface oxides or hydroxides) and undergo partial dissolution in the liquid phase under dark conditions, such Ni and Cu oxidized and dissolved species are reduced/redeposited as a bimetallic NiCu phase at the TiO2 surface under illumination. The dissolution/redeposition mechanism is triggered by TiO2 conduction band electrons. We not only prove a UV-light-induced healing of the NiCu co-catalyst but also unambiguously demonstrate that the species responsible for the strongly enhanced photocatalytic H2 evolution of NiCu nanoparticles are the metallic states of Ni and Cu.
AB - Cu- or Ni-decorated semiconductors represent a potential low-cost alternative to noble-metal-modified photocatalysts. Even more effective are bimetallic NiCu nanoparticles, which can provide a remarkable photocatalytic H2 evolution enhancement compared to single-element Cu or Ni systems. The main concern of such alloyed co-catalysts is their activity with respect to alteration of their elemental composition and oxidation state over reaction time. Ex situ characterization techniques provide controversial interpretations of the co-catalytic role of the individual elements. Hypotheses such as the in situ reduction of “native” Ni or Cu species during photocatalysis, the oxidation of metallic Cu or Ni into oxides or hydroxides, or the formation of p-n junctions or core/shell structures have been proposed. Herein, we present an operando X-ray absorption spectroscopy study of a NiCu-TiO2 system under UV light illumination in ethanol-water solutions, i.e., under photocatalytic H2 evolution conditions. The experimental approach allows for monitoring in real time chemical changes that take place in the co-catalyst under intermittent illumination, i.e., under light on-off cycles. We show that while Ni and Cu are partially oxidized in the as-formed NiCu co-catalyst (air-formed surface oxides or hydroxides) and undergo partial dissolution in the liquid phase under dark conditions, such Ni and Cu oxidized and dissolved species are reduced/redeposited as a bimetallic NiCu phase at the TiO2 surface under illumination. The dissolution/redeposition mechanism is triggered by TiO2 conduction band electrons. We not only prove a UV-light-induced healing of the NiCu co-catalyst but also unambiguously demonstrate that the species responsible for the strongly enhanced photocatalytic H2 evolution of NiCu nanoparticles are the metallic states of Ni and Cu.
KW - In situ XAS
KW - NiCu alloy nanoparticles
KW - Photocatalytic H evolution
KW - Solid-state dewetting
KW - TiO nanotubes
KW - NLA
UR - http://www.scopus.com/inward/record.url?scp=85090974452&partnerID=8YFLogxK
U2 - 10.1021/acscatal.0c01373
DO - 10.1021/acscatal.0c01373
M3 - Article
AN - SCOPUS:85090974452
SN - 2155-5435
VL - 10
SP - 8293
EP - 8302
JO - ACS catalysis
JF - ACS catalysis
IS - 15
ER -