2022
DOI: 10.1103/physrevb.105.134416
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Origin of perpendicular magnetic anisotropy in CoxFe3xO4+δ thin films studied by x-ray magnetic circular and linear dichroi

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Cited by 7 publications
(7 citation statements)
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“…In this case, the direction of strain and enhanced orbital moments are orthogonal in principle. Similar scenario can be adopted to the perpendicular MCA in Co-ferrite CoFe 2 O 4 as orbitalelastic effect in Co 2+ site with large orbital moment [75]. Second type can be understood as quadrupole cases; the direction of strain becomes an easy axis.…”
Section: Discussionmentioning
confidence: 90%
“…In this case, the direction of strain and enhanced orbital moments are orthogonal in principle. Similar scenario can be adopted to the perpendicular MCA in Co-ferrite CoFe 2 O 4 as orbitalelastic effect in Co 2+ site with large orbital moment [75]. Second type can be understood as quadrupole cases; the direction of strain becomes an easy axis.…”
Section: Discussionmentioning
confidence: 90%
“…Large XMCD signals in the Co L edge correspond to contribution of the orbital moment through the distorted Co 2+ (3d 7 ) O h site. 25,26 The Pt growth-temperature dependence of XMCD indicates the stability of Co x Fe 3−x O 4 /Pt interface structures between CFO/Pt@500 and CFO/Pt@600, except for the peak intensity ratio of Fe 2+ (O h ) components (Figure 2b). Since XAS and XMCD spectra in the TEY probe down to a depth of less than 3 nm from the sample surface, the interfacial regions can be detected clearly.…”
Section: Resultsmentioning
confidence: 99%
“…The shapes of hysteresis curves are different between 500 and 600 °C, which is consistent with the SQUID measurements. Large XMCD signals in the Co L edge correspond to contribution of the orbital moment through the distorted Co 2+ (3d 7 ) O h site. , …”
Section: Resultsmentioning
confidence: 99%
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