Welcome to the new version of CaltechAUTHORS. Login is currently restricted to library staff. If you notice any issues, please email coda@library.caltech.edu
Published October 21, 2024 | Supplemental Material
Journal Article Open

The spectroscopy of hydride in single crystals of SrTiO₃ perovskite

  • 1. ROR icon California Institute of Technology

Abstract

Under reducing conditions, SrTiO3 perovskite can exchange up to 20% of its O2− ions for H (hydride), greatly influencing its material properties. This not only presents intriguing possibilities for material design, but also for hydrogen sequestration in the deep earth, where perovskite-structured minerals are abundant. However, uncertainties remain surrounding hydride incorporation in SrTiO3, including details of the hydride structural state, and how hydride interacts with the broader defect chemistry of SrTiO3. Additionally, experimental studies of hydride in SrTiO3 and other perovskites may face analytical limitations. The most common methods for characterizing hydride, namely 1H NMR, may not be suitable in all experimental contexts, including materials with relatively low hydride concentrations and in situ high-pressure, high-temperature experiments. Here, we present an investigation of hydride in single crystals of SrTiO3 focused on detailed spectroscopic measurements. Through a combination of density functional theory (DFT)-assisted Fourier transform infrared (FTIR) spectroscopy and UV-vis spectroscopy, we observe structural hydride and its effects on the electronic transitions in SrTiO3. These results are compared directly against 1H NMR. We find that, although hydride is sometimes difficult to identify via FTIR, infrared spectroscopy is significantly more sensitive to hydride than 1H NMR. We also find that DFT makes accurate predictions about the spectroscopic behavior of hydride in SrTiO3, pointing to the value of ab initio techniques in future studies.

Copyright and License

© the Owner Societies 2024

Acknowledgement

The authors thank Dr Channing Ahn and Dr Cullen Quine for providing access to facilities necessary for sample preparation. W. A. G. thanks NSF (CBET 2311117) for support. G. R. R. thanks NSF (EAR-2149559).

Data Availability

The data supporting this article have been included as part of the ESI.

Contributions

Conceptualization: W. R. P.; formal analysis: W. R. P.; funding acquisition: W. A. G., G. R. R.; investigation: W. R. P., S. J. H.; methodology: W. R. P.; supervision: W. A. G., G. R. R.; writing – original draft: W. R. P.; writing – review & editing: W. R. P., S. J. H., W. A. G., G. R. R.

Files

d4cp02852j1.pdf
Files (821.3 kB)
Name Size Download all
md5:b6e3079cc2e0da32b243c4a920f6384b
821.3 kB Preview Download

Additional details

Created:
November 21, 2024
Modified:
November 21, 2024