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On the ‘centre of gravity’ method for measuring the composition of magnetite/maghemite mixtures, or the stoichiometry of magnetite-maghemite solid solutions, via57Fe Mössbauer spectroscopy
Author(s) -
Jeppe Fock,
Lara K. Bogart,
David GonzálezAlonso,
J.I. Espeso,
Mikkel Fougt Hansen,
Miriam Varón,
Cathrine Frandsen,
Quentin A. Pankhurst
Publication year - 2017
Publication title -
journal of physics d applied physics
Language(s) - English
Resource type - Journals
eISSN - 1361-6463
pISSN - 0022-3727
DOI - 10.1088/1361-6463/aa73fa
Subject(s) - maghemite , magnetite , mössbauer spectroscopy , stoichiometry , solid solution , materials science , analytical chemistry (journal) , chemistry , mineralogy , crystallography , metallurgy , chromatography
We evaluate the application of 57Fe Mossbauer spectroscopy to the determination of the composition of magnetite (Fe3O4)/maghemite (γ-Fe2O3) mixtures and the stoichiometry of magnetite-maghemite solid solutions. In particular, we consider a recently proposed model-independent method which does not rely on a priori assumptions regarding the nature of the sample, other than that it is free of other Fe-containing phases. In it a single parameter, δRT—the ‘centre of gravity’, or area weighted mean isomer shift at room temperature, T = 295 ± 5 K—is extracted by curve-fitting a sample’s Mossbauer spectrum, and is correlated to the sample’s composition or stoichiometry. We present data on highpurity magnetite and maghemite powders, and mixtures thereof, as well as comparison literature data from nanoparticulate mixtures and solid solutions, to show that a linear correlation exists between δRT and the numerical proportion of Fe atoms in the magnetite environment: α = Femagnetite/Fetotal = − ( ) δ δ RT o /m, where δo = 0.3206 ± 0.0022mm s−1 and m = 0.2135 ± 0.0076mm s−1 . We also present equations to relate α to the weight percentage w of magnetite in mixed phases, and the magnetite stoichiometry x = Fe2+/Fe3+ in solid solutions. The analytical method is generally applicable, but is most accurate when the absorption profiles are sharp; in some samples this may require spectra to be recorded at reduced temperatures. We consider such cases and provide equations to relate δ ( ) T to the corresponding α value.

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