2024
Profiles of oxygen and titanium point defects in ferromagnetic TiO2 films
TRAN, Quynh Nhu Thi, Martin FRIÁK, Ivana MIHÁLIKOVÁ, Michal KIABA, Hoa Hong NGUYEN et. al.Základní údaje
Originální název
Profiles of oxygen and titanium point defects in ferromagnetic TiO2 films
Autoři
TRAN, Quynh Nhu Thi (704 Vietnam, domácí), Martin FRIÁK (203 Česká republika, domácí), Ivana MIHÁLIKOVÁ (703 Slovensko, domácí), Michal KIABA (703 Slovensko, domácí) a Hoa Hong NGUYEN (250 Francie, garant, domácí)
Vydání
Journal of Physics D: Applied Physics, IOP Publishing Ltd, 2024, 0022-3727
Další údaje
Jazyk
angličtina
Typ výsledku
Článek v odborném periodiku
Obor
10302 Condensed matter physics
Stát vydavatele
Velká Británie a Severní Irsko
Utajení
není předmětem státního či obchodního tajemství
Odkazy
Impakt faktor
Impact factor: 3.400 v roce 2022
Organizační jednotka
Přírodovědecká fakulta
UT WoS
001196338000001
Klíčová slova anglicky
vacancies; defects; ferromagnetic; DMSO; spintronics
Štítky
Příznaky
Mezinárodní význam, Recenzováno
Změněno: 16. 4. 2024 11:03, Mgr. Marie Šípková, DiS.
Anotace
V originále
Experimentally it is shown that without any oxygen manipulation for TiO2, a strong room temperature ferromagnetism could be expected only in ultra-thin films, with the ideal thickness below 100 nm. Both bulks and nano-powders of TiO2 are diamagnetic, indicating that the surface and its nano-sublayers play very important roles in tailoring the magnetic properties in this type of compound. To shed a new light on the defect-related magnetism in the typical case of anatase TiO2 surfaces, we have performed a series of quantum-mechanical calculations for TiO2 slabs containing Ti or O vacancies in different distances from the (001) surface. The lowest formation energies were obtained for the Ti vacancies in the first sub-surface layer and the O vacancies within the surface. The computed magnetic states reflect complicated structural relaxations of atoms influenced by both the surface and vacant atomic positions. O atoms cannot contribute much to magnetic moment when Ti vacancies are isolated and far from the surface. Ti vacancies in TiO2 are only metastable. The formation energy of Ti interstitials is lower than for Ti vacancies since high-temperature annealing, especially with a lot of O2 available that would fill up O-related defects, and as a result, eliminate most of Ti vacancies. Lower temperatures, less O2, and shorter exposure times may enable not only partial elimination of Ti vacancies but also can facilitate their diffusion into different states of aggregations. In the ferromagnetic films (i.e. thin films below 100 nm), it looks like that the O atoms are located closer to the Ti vacancies.
Návaznosti
EH22_008/0004572, projekt VaV |
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GA22-21547S, projekt VaV |
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90110, velká výzkumná infrastruktura |
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90140, velká výzkumná infrastruktura |
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