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Magnetic Oxide Heterostructures: EuO on Cubic Oxides ... - JuSER
Magnetic Oxide Heterostructures: EuO on Cubic Oxides ... - JuSER
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5.1. Chemical stabilization of bulk-like EuO directly on silicon 91<br />
HAXPES: Analysis of the Eu 3d deep core-levels<br />
Now we proceed with spectra of the more deeply bound Eu 3d core-levels, which helps to<br />
provide a consistent quantification of the initial state valency in conjunction with the Eu 4f<br />
results. We note, that analyzing the 3d core-level spectra has a significant advantage for the<br />
determination of the initial state Eu valency compared e. g. to the 4d core-levels, because the<br />
3d states show a much weaker multiplet splitting and larger photoexcitation cross section.<br />
Moreover, the kinetic energy of Eu 3d photoelectrons is reduced by about 1150 eV, thus the<br />
probe is more surface sensitive within the EuO layer, as sketched in Fig 5.2.<br />
Eu 3d photoemission spectra for EuO compounds (i) and (ii), recorded in normal emission<br />
geometry, are depicted in Fig. 5.3f and h. The spectra consist of a main peaks, the spin–orbitlike<br />
final state groups 3d j= 5/2 and 3d j= 3/2, which are clearly separated by a large spin–orbit<br />
coupling of 29.2 eV in agreement with previous studies. 159 The broad structure in the center<br />
is assigned to extrinsic plasmon excitations caused by high energy 3d photoelectrons, which<br />
dissipate the plasmon energy in the electron gas of the metallic Al top layer. 173 The plasmons<br />
are located at the expected energy loss (16 eV) from the 3d5/2 peak and the 3d3/2 peak.<br />
Stoichiometric EuO (i) shows one main peak in each of the Eu 3d5/2 and 3d3/2 groups in Fig. 5.3f.<br />
Within the two spin–orbit split groups, the distribution of final states m J is asymmetrically<br />
shaped, in perfect agreement with theoretical calculations of the divalent Eu 3d multiplet,<br />
as depicted for comparison in Fig. 5.3j. 110 A satellite peak in the high binding energy region<br />
of the Eu 3d5/2 (and 3d3/2) multiplet separated by 7.8 eV (6.3 eV) from the main peak belongs<br />
to the divalent Eu 2+ multiplet of the 3d 9 4f 7 final state. Energy splitting as well as intensity<br />
ratios of the satellites agree with previous reports on calculated and measured multiplet<br />
spectra of divalent Eu compounds. 110,111<br />
Evaluating the oxygen-rich EuO compound (ii) inFig.5.3h, we observe prominent double<br />
peak structures in the 3d5/2 (3d3/2) regions, which are separated by 10.45 eV (10.90 eV). We<br />
assign these features to divalent Eu 2+ (3d 9 4f 7 final state) and trivalent Eu 3+ (3d 9 4f 6 final<br />
state) spectral contributions. Similar with the divalent Eu structure, the Eu 3+ 3d multiplet<br />
consists of a doublet whith a satellite peak appearing at 6.9 eV higher binding energy below<br />
the 3d5/2 main peak. The Eu 3+ 3d3/2 satellite structure is broadly distributed (not shown). The<br />
energy positions and shape of the Eu 2+ and Eu 3+ 3d multiplet final states agree well with<br />
previous experiments 176,180,181 and theoretical calculations, 110,111 as illustrated in Fig. 5.3j.<br />
For a depth-sensitive analysis of the 3d core-levels, we calculate the energy and angle-depen-<br />
Table 5.1.: Binding energies E B and Eu 3+ valency ratios r Eu3+ for (i) stoichiometric EuO and (ii) oxygenrich<br />
Eu 1 O 1+x , as obtained by least-squares fitting of the Eu 4f and 3d spectra.<br />
Eu 4f<br />
EB<br />
Eu2+<br />
EB<br />
Eu3+<br />
r Eu3+<br />
4f<br />
(i) EuO 1.8 eV 7.0–11.1 eV 7.4 ± 1.2%<br />
(ii) EuO 1+x 1.64 eV 7.0–11.1 eV 66 ± 2%<br />
Eu 3d<br />
EB Eu2+ (eV) EB Eu3+ (eV) r3d<br />
Eu3+<br />
j = 5/2 3/2 E SO 5/2 3/2 E SO 5/2 3/2<br />
(i) EuO 1124.9 1154.1 29.2 1134.7 1164.4 29.7 4.1% 3.2%<br />
(ii) EuO 1+x 1125.0 1154.3 29.3 1134.8 1164.5 29.7 59% 49%