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Magnetic Oxide Heterostructures: EuO on Cubic Oxides ... - JuSER

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70 4. Results I: Single-crystalline epitaxial EuO thin films on cubic oxides<br />

(a)<br />

160x10 3<br />

intensity (counts)<br />

110<br />

60<br />

bulk vs. ultrathin EuO on cYSZ(001)<br />

Eu 3d hv=5.9 keV, normal emission,<br />

dE=0.2 eV, T=63 K<br />

Eu 2+ 3d 3/2<br />

ultrathin (1 nm) EuO<br />

bulk-like (4 nm) EuO<br />

Si<br />

plasmon<br />

(Eu 3+ )<br />

Eu 2+ 3d 5/2<br />

1160 1150 1140 1130 1120<br />

binding energy (eV)<br />

(b)<br />

bulk vs. ultrathin EuO on cYSZ(001)<br />

50x10 3 hv=5.9 keV, normal emission,<br />

dE=0.2 eV, T=63 K<br />

intensity (counts)<br />

30<br />

Eu 4d<br />

ultrathin (1 nm) EuO<br />

bulk-like (4 nm) EuO<br />

7<br />

DJ<br />

(J=1..5)<br />

9<br />

DJ<br />

(J=2..6)<br />

145 140 135 130 125<br />

binding energy (eV)<br />

Figure 4.12.: HAXPES of ultrathin single-crystalline EuO/cYSZ (100) recorded at 63 K. Large crosssections<br />

of Eu 3d and 4d levels in (a) and (b) permit one to resolve even small intensity changes<br />

in the multiplet structure.<br />

peaks at low binding energy, as depicted in Fig. 4.11c. They resolve a complex multiplet<br />

structure. The 4d orbital shares the same principal quantum number with the 4f valence<br />

level which involves a strong d–f exchange interaction due to radial overlap. Therefore, we<br />

cannot separate 4d spectra into 4d J=3/2 and 4d J=5/2 components, but rather to a J = L − S<br />

multiplet splitting, and assign the peaks to the 7 D J and 9 D J multiplets, respectively. 114,115<br />

Eu 4d final states are well described by the intermediate coupling scheme (LSJ) in which<br />

both spin-orbit and exchange splitting are treated as perturbations. 112 This leads to an intensity<br />

ratio of about 1:3 for the septet to the nonet peaks 161 of the final state configuration<br />

∣<br />

∣4f 7 : S7/2〉∣ 8 ∣∣4d<br />

〉∣ 9 : 9 D J , 7 D ∣∣ɛl<br />

〉<br />

J . Once more, we observe a clear Eu 2+ valency in EuO, indicative<br />

for the integral divalent state of EuO.<br />

In the HAXPES spectrum (Fig. 4.11c), the fine structure of the 7 D final state is not resolved,<br />

whereas the J = 2–6 components in the 9 D state are easily identified. Energy losses due to<br />

the excitation of the 5p or the 4f electrons during photoemission are predicted to lead to<br />

satellites at 5–10 eV higher binding energy from the main line. 162 . Furthermore, smaller<br />

contributions of the 7 D final state exist at up to 20 eV higher binding energy than the 7 D<br />

main peak. 114 However, these higher binding energy features overlap within intensities of<br />

an extrinsic plasmon of silicon and the background of inelastic electron scattering.<br />

In a further step, we investigate the two core-levels from ultrathin single-crystalline EuO, and<br />

compare a bulk-like EuO thin film (4 nm) with a quasi-two dimensional EuO layer (1 nm).<br />

Such thicknesses are typical for tunnel barriers in future spin-selective tunnel contacts. In<br />

Fig. 4.12a, b, the HAXPES spectra of Eu 3d and Eu 4d core-levels are taken at LN 2 temperature<br />

in order to reduce thermal broadening. We observe a line shape of the core-level spectra<br />

comparable with thicker EuO, even the multiplet splitting originating from the single atomic<br />

angular momenta J is resolved with an identical distribution of spectral weight.<br />

In the spectra of 1 nm EuO, a small deviation can be observed at 8 eV shift towards higher<br />

binding energy with respect to the main multiplet features. We observe this small feature<br />

consistently in both the Eu 3d and 4d spectra, and identify this as chemical shift of Eu 3+<br />

ions. 1 An explanantion may be ionic oxygen provided by the cYSZ substrate, to which the<br />

ultrathin EuO layer reacts sensitively with oxidation.<br />

In conclusion, we investigated Eu core-levels of heterostructures with single-crystalline EuO<br />

thin films in the range 1–20 nm by HAXPES. We selected the Eu 3d and the 4d orbitals for

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