Significant Oxygen Underestimation When Quantifying Barium-Doped SrTiO Layers by Atom Probe Tomography.

atom probe tomography barium-doped strontium titanate composition quantification energy elastic recoil diffraction oxygen underestimation perovskites rutherford backscattering spectroscopy

Journal

Microscopy and microanalysis : the official journal of Microscopy Society of America, Microbeam Analysis Society, Microscopical Society of Canada
ISSN: 1435-8115
Titre abrégé: Microsc Microanal
Pays: England
ID NLM: 9712707

Informations de publication

Date de publication:
17 Jan 2024
Historique:
received: 12 06 2023
revised: 05 12 2023
accepted: 22 12 2023
medline: 17 1 2024
pubmed: 17 1 2024
entrez: 17 1 2024
Statut: aheadofprint

Résumé

In this paper, the capability for quantifying the composition of Ba-doped SrTiO layers from an atom probe measurement was explored. Rutherford backscattering spectrometry and time-of-flight/energy elastic recoil detection were used to benchmark the composition where the amount of titanium was intentionally varied between samples. The atom probe results showed a significant divergence from the benchmarked composition. The cause was shown to be a significant oxygen underestimation (≳14 at%). The ratio between oxygen and titanium for the samples varied between 2.6 and 12.7, while those measured by atom probe tomography were lower and covered a narrower range between 1.4 and 1.7. This difference was found to be associated with the oxygen and titanium predominantly field evaporating together as a molecular ion. The evaporation fields and bonding chemistries determined showed inconsistencies for explaining the oxygen underestimation and ion species measured. The measured ion charge state was in excellent agreement with that predicted by the Kingham postionization theory. Only by considering the measured ion species, their evaporation fields, the coordination chemistry, the analysis conditions, and some recently reported density functional theory modeling for oxide field emission were we able to postulate a field emission and oxygen neutral desorption process that may explain our results.

Identifiants

pubmed: 38232229
pii: 7564694
doi: 10.1093/micmic/ozad144
pii:
doi:

Types de publication

Journal Article

Langues

eng

Sous-ensembles de citation

IM

Informations de copyright

© The Author(s) 2024. Published by Oxford University Press on behalf of the Microscopy Society of America. All rights reserved. For permissions, please e-mail: journals.permissions@oup.com.

Auteurs

Richard J H Morris (RJH)

imec, Kapeldreef 75, Leuven 3001, Belgium.

Jhao-Rong Lin (JR)

imec, Kapeldreef 75, Leuven 3001, Belgium.
Department of Physics and Astronomy, Quantum Solid-State Physics, KU Leuven, Celestijnenlaan 200D, Leuven B-3001, Belgium.

Jeroen E Scheerder (JE)

imec, Kapeldreef 75, Leuven 3001, Belgium.

Mihaela I Popovici (MI)

imec, Kapeldreef 75, Leuven 3001, Belgium.

Johan Meersschaut (J)

imec, Kapeldreef 75, Leuven 3001, Belgium.

Ludovic Goux (L)

imec, Kapeldreef 75, Leuven 3001, Belgium.

Gouri Sankar Kar (GS)

imec, Kapeldreef 75, Leuven 3001, Belgium.

Paul van der Heide (P)

imec, Kapeldreef 75, Leuven 3001, Belgium.

Claudia Fleischmann (C)

imec, Kapeldreef 75, Leuven 3001, Belgium.
Department of Physics and Astronomy, Quantum Solid-State Physics, KU Leuven, Celestijnenlaan 200D, Leuven B-3001, Belgium.

Classifications MeSH