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Profiles of oxygen and titanium point defects in ferromagnetic TiO2 films

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68081723%3A_____%2F24%3A00584888" target="_blank" >RIV/68081723:_____/24:00584888 - isvavai.cz</a>

  • Alternative codes found

    RIV/00216224:14310/24:00135763

  • Result on the web

    <a href="https://iopscience.iop.org/article/10.1088/1361-6463/ad3767" target="_blank" >https://iopscience.iop.org/article/10.1088/1361-6463/ad3767</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1088/1361-6463/ad3767" target="_blank" >10.1088/1361-6463/ad3767</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Profiles of oxygen and titanium point defects in ferromagnetic TiO2 films

  • Original language description

    Experimentally it is shown that without any oxygen manipulation for TiO2, a strong roomntemperature ferromagnetism could be expected only in ultra-thin films, with the ideal thicknessnbelow 100 nm. Both bulks and nano-powders of TiO2 are diamagnetic, indicating that thensurface and its nano-sublayers play very important roles in tailoring the magnetic properties innthis type of compound. To shed a new light on the defect-related magnetism in the typical casenof anatase TiO2 surfaces, we have performed a series of quantum-mechanical calculations fornTiO2 slabs containing Ti or O vacancies in different distances from the (001) surface. Thenlowest formation energies were obtained for the Ti vacancies in the first sub-surface layer andnthe O vacancies within the surface. The computed magnetic states reflect complicated structuralnrelaxations of atoms influenced by both the surface and vacant atomic positions. O atoms cannotncontribute much to magnetic moment when Ti vacancies are isolated and far from the surface.nTi vacancies in TiO2 are only metastable. The formation energy of Ti interstitials is lower thannfor Ti vacancies since high-temperature annealing, especially with a lot of O2 available thatnwould fill up O-related defects, and as a result, eliminate most of Ti vacancies. Lowerntemperatures, less O2, and shorter exposure times may enable not only partial elimination of Tinvacancies but also can facilitate their diffusion into different states of aggregations. In thenferromagnetic films (i.e. thin films below 100 nm), it looks like that the O atoms are locatedncloser to the Ti vacancies.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • OECD FORD branch

    10302 - Condensed matter physics (including formerly solid state physics, supercond.)

Result continuities

  • Project

    Result was created during the realization of more than one project. More information in the Projects tab.

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2024

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Name of the periodical

    Journal of Physics D-Applied Physics

  • ISSN

    0022-3727

  • e-ISSN

    1361-6463

  • Volume of the periodical

    57

  • Issue of the periodical within the volume

    26

  • Country of publishing house

    GB - UNITED KINGDOM

  • Number of pages

    8

  • Pages from-to

    265302

  • UT code for WoS article

    001196338000001

  • EID of the result in the Scopus database

    2-s2.0-85189824930