Published June 5, 2018 | Version Published + Supplemental Material
Journal Article Open

Synergy between Fe and Ni in the optimal performance of (Ni,Fe)OOH catalysts for the oxygen evolution reaction

  • 1. ROR icon California Institute of Technology
  • 2. ROR icon Joint Center for Artificial Photosynthesis

Abstract

The oxygen evolution reaction (OER) is critical to solar production of fuels, but the reaction mechanism underlying the performance for a best OER catalyst, Fe-doped NiOOH [(Ni,Fe)OOH], remains highly controversial. We used grand canonical quantum mechanics to predict the OER mechanisms including kinetics and thus overpotentials as a function of Fe content in (Ni,Fe)OOH catalysts. We find that density functional theory (DFT) without exact exchange predicts that addition of Fe does not reduce the overpotential much. However, DFT with exact exchange predicts dramatic improvement in performance for (Ni,Fe)OOH, leading to an overpotential of 0.42 V and a Tafel slope of 23 mV/decade (dec), in good agreement with experiments, 0.3–0.4 V and 30 mV/dec. We reveal that the high spin d^4 Fe(IV) leads to efficient formation of an active O radical intermediate, while the closed shell d^6 Ni(IV) catalyzes the subsequent O–O coupling, and thus it is the synergy between Fe and Ni that delivers the optimal performance for OER.

Additional Information

© 2018 National Academy of Sciences. Published under the PNAS license. Contributed by William A. Goddard III, April 14, 2018 (sent for review December 18, 2017; reviewed by Daniel G. Nocera and Annabella Selloni) PNAS May 21, 2018. 201722034; published ahead of print May 21, 2018. https://doi.org/10.1073/pnas.1722034115 This work was supported by the Joint Center for Artificial Photosynthesis, a Department of Energy (DOE) Energy Innovation Hub, supported through the Office of Science of the DOE under Award DE-SC0004993. The calculations were carried out on the Extreme Science and Engineering Discovery Environment, which is supported by National Science Foundation Grant ACI-1053575, and the Zwicky Astrophysics Supercomputer at Caltech. Author contributions: H.X. and W.A.G. designed research; H.X. and H.S. performed research; H.X. and H.S. analyzed data; and H.X. and W.A.G. wrote the paper. Reviewers: D.G.N., Harvard University; and A.S., Princeton University. The authors declare no conflict of interest. This article contains supporting information online at www.pnas.org/lookup/suppl/doi:10.1073/pnas.1722034115/-/DCSupplemental.

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Additional details

Identifiers

PMCID
PMC6003342
Eprint ID
86530
DOI
10.1073/pnas.1722034115
Resolver ID
CaltechAUTHORS:20180521-155521778

Related works

Funding

Joint Center for Artificial Photosynthesis (JCAP)
Department of Energy (DOE)
DE-SC0004993
NSF
ACI-1053575

Dates

Created
2018-05-21
Created from EPrint's datestamp field
Updated
2021-11-15
Created from EPrint's last_modified field

Caltech Custom Metadata

Caltech groups
JCAP
Other Numbering System Name
WAG
Other Numbering System Identifier
1286