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- W1966035443 endingPage "1825" @default.
- W1966035443 startingPage "1823" @default.
- W1966035443 abstract "A variety of rutile samples were heat treated in atmospheres of ${mathrm{H}}_{2}$, ${mathrm{H}}_{2}$O, and ${mathrm{O}}_{2}$ according to prescriptions which theoretically and experimentally either favor or suppress H interstitial formation. The H concentration and conduction-electron concentrations in the samples were monitored optically. The $A$ spectrum, which has been universally accepted as being due to ${mathrm{Ti}}^{3+}$ interstitials, is found instead to be associated with H." @default.
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- W1966035443 date "1974-09-01" @default.
- W1966035443 modified "2023-09-23" @default.
- W1966035443 title "Reinterpretation of the <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML display=inline><mml:mrow><mml:msup><mml:mrow><mml:mi mathvariant=normal>Ti</mml:mi></mml:mrow><mml:mrow><mml:mn>3</mml:mn><mml:mo>+</mml:mo></mml:mrow></mml:msup></mml:mrow></mml:math>interstitial electron-spin-resonance spectrum in rutile" @default.
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- W1966035443 doi "https://doi.org/10.1103/physrevb.10.1823" @default.
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