4.5 Article

Reduced synthesis temperatures of SrNbO2 N perovskite films for photoelectrochemical fuel production

Journal

JOURNAL OF MATERIALS RESEARCH
Volume 37, Issue 2, Pages 424-435

Publisher

SPRINGER HEIDELBERG
DOI: 10.1557/s43578-021-00448-3

Keywords

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Funding

  1. US Department of Energy (DOE) [DE-AC36-08GO28308]
  2. Office of Energy Efficiency and Renewable Energy (EERE) Hydrogen and Fuel Cell Technologies Office (HFTO), as a part of HydroGEN Energy Materials Network (EMN) consortium
  3. Office of Science, Basic Energy Sciences, as a part of HydroGEN Energy Materials Network (EMN) consortium (annealing optimization and electron microscopy)
  4. DOE-SC-BES [DE-AC02-76SF00515]
  5. Office of Science, Basic Energy Sciences, part of Fuels from Sunlight Hubs Joint Center for Artificial Photosynthesis
  6. Office of Science, Basic Energy Sciences, part of Liquid Sunlight Alliance (SDC design, PEC characterization)

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This study reports reduced synthesis temperatures for SrNbO2N perovskite thin films on Si substrates, and investigates the impact of different chemical compositions on their photocurrent density.
Perovskite oxynitrides, such as SrNbO2N, have been shown to be promising materials for photoanodes in tandem photoelectrochemical cells, due to their suitable bandgap and charge transport. However, thin film synthesis and characterization of oxynitride perovskites are challenging due to high processing temperatures that are incompatible with available substrates. In this work, we report on reduced synthesis temperatures of SrNbO2N perovskite thin films on Si substrates across a range of chemical compositions. Polycrystalline thin films with perovskite crystal structure are obtained by sputtering at ambient temperature and annealing at 550-600 degrees C. The perovskite structure has a relatively broad range of cation composition between 50 and 60% Sr with varying O/N ratio according to Rutherford backscattering spectrometry. The maximum photocurrent density was obtained at 55 cation % of Sr, which is slightly Sr-rich compared to the nominal SrNbO2N stoichiometry.This work shows the importance of considering cation and anion composition in studying oxynitride perovskites for solar fuel applications.

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