Unravelling the origin of ultra-low conductivity in SrTiO Thin films. Sr vacancies and Ti on A-sites cause Fermi level pinning
Creators
- Morgenbesser, Maximilian1
- Viernstein, Alexander1
- Schmid, Alexander1
- Herzig, Christopher1
- Kubicek, Markus1
- Taibl, Stefanie1
- Limbeck, Andreas1
- Fleig, Jürgen1
- Bimashofer, Gesara2, 3
- Stahn, Jochen3
- Fernandes Vaz, Carlos Antonio4, 3
- Döbeli, Max5
- Biautti, Federico6
- Dios Sirvent, Juan de6
- Liedke, Maciej Oskar7
- Butterling, Maik7
- Wagner, Andreas7
- Kamiński, Michał8
- Tolkiehn, Martin8
- Vonk, Vedran8
- Stierle, Andreas9, 8
- Tarancon, Albert10, 6
- 1. Institute of Chemical Technologies and Analytics, Vienna, 1060 (Austria)
- 2. Swiss Light Source, Paul Scherrer Institut, Villingen, CH‐5232 (Switzerland)
- 3. Laboratory for Neutron Scattering and Imaging, Paul Scherrer Institut, Villingen, 5232 (Switzerland)
- 4. Department of Chemistry and Applied Biosciences, ETH Zürich, Zurich, 8092 (Switzerland)
- 5. Laboratory of Ion Beam Physics, ETH Zürich, Zürich, 8093 (Switzerland)
- 6. Catalonia Institute for Energy Research (IREC), Barcelona, 08930 (Spain)
- 7. Institute of Radiation Physics, Helmholtz‐Zentrum Dresden‐Rossendorf, Dresden, 01328 (Germany)
- 8. Deutsches Elektronen Synchrotron (DESY), Hamburg, D‐22607 (Germany)
- 9. Fachbereich Physik, Universität Hamburg, Hamburg, 22607 (Germany)
- 10. Catalan Institution for Research and Advanced Studies (ICREA), Barcelona, 08930 (Spain)
Description
Different SrTiO thin films are investigated to unravel the nature of ultra-low conductivities recently found in SrTiO films prepared by pulsed laser deposition. Impedance spectroscopy reveals electronically pseudo-intrinsic conductivities for a broad range of different dopants (Fe, Al, Ni) and partly high dopant concentrations up to several percent. Using inductively-coupled plasma optical emission spectroscopy and reciprocal space mapping, a severe Sr deficiency is found and positron annihilation lifetime spectroscopy revealed Sr vacancies as predominant point defects. From synchrotron-based X-ray standing wave and X-ray absorption spectroscopy measurements, a change in site occupation is deduced for Fe-doped SrTiO films, accompanied by a change in the dopant type. Based on these experiments, a model is deduced, which explains the almost ubiquitous pseudo-intrinsic conductivity of these films. Sr deficiency is suggested as key driver by introducing Sr vacancies and causing site changes (Fe and Ti) to accommodate nonstoichiometry. Sr vacancies act as mid-gap acceptor states, pinning the Fermi level, provided that additional donor states (most probably Ti) are present. Defect chemical modeling revealed that such a Fermi level pinning also causes a self-limitation of the Ti site change and leads to a very robust pseudo-intrinsic situation, irrespective of Sr/Ti ratios and doping. (© 2022 The Authors. Advanced Functional Materials published by Wiley‐VCH GmbH)
Availability note (English)
Available from: http://dx.doi.org/10.1002/adfm.202202226Additional details
Identifiers
Publishing Information
- Journal Title
- Advanced Functional Materials (Internet)
- Journal Volume
- 32
- Journal Issue
- 38
- Journal Page Range
- p. 1-20
- ISSN
- 1616-3028
- CODEN
- AFMDC6
INIS
- Country of Publication
- Germany
- Country of Input or Organization
- Germany
- INIS RN
- 53115523
- Subject category
- S75: CONDENSED MATTER PHYSICS, SUPERCONDUCTIVITY AND SUPERFLUIDITY;
- Descriptors DEI
- ABSORPTION SPECTROSCOPY; ALUMINIUM; DOPED MATERIALS; ELECTRIC CONDUCTIVITY; EMISSION SPECTROSCOPY; ENERGY BEAM DEPOSITION; FERMI LEVEL; IRON; LASER RADIATION; NICKEL; STRONTIUM TITANATES; THIN FILMS; VACANCIES
- Descriptors DEC
- ALKALINE EARTH METAL COMPOUNDS; CRYSTAL DEFECTS; CRYSTAL STRUCTURE; DEPOSITION; ELECTRICAL PROPERTIES; ELECTROMAGNETIC RADIATION; ELEMENTS; ENERGY LEVELS; FILMS; MATERIALS; METALS; OXYGEN COMPOUNDS; PHYSICAL PROPERTIES; POINT DEFECTS; RADIATIONS; SPECTROSCOPY; STRONTIUM COMPOUNDS; SURFACE COATING; TITANATES; TITANIUM COMPOUNDS; TRANSITION ELEMENT COMPOUNDS; TRANSITION ELEMENTS
Optional Information
- Notes
- AID: 2202226