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Magnetic Oxide Heterostructures: EuO on Cubic Oxides ... - JuSER
Magnetic Oxide Heterostructures: EuO on Cubic Oxides ... - JuSER
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48 3. Experimental details<br />
coordinates q i are converted into real space distances with Miller’s indices m i ,<br />
⎧<br />
d i = 1 ⎪⎨ h or k, for i parallel,<br />
·m<br />
q i , m i =<br />
i<br />
⎪⎩ l, for i perpendicular.<br />
(3.9)<br />
In this work, all X-ray diffraction experiments are conducted with a four-cycle Phillips MRD<br />
Pro using monochromatized Cu Kα radiation.<br />
3.4.3. Hard X-ray photoemission spectroscopy (HAXPES)<br />
Quantifying the element-specific electronic properties of a multilayer system is impossible<br />
when using surface-sensitive soft X-ray photoemission due to its limited probing depth. The<br />
major limiting factor is the inelastic scattering of free electrons in solids. For an electron with<br />
energy E kin = 2 k 2<br />
2m , the inelastic mean free path (IMFP) can be expressed as λ = ( )<br />
k<br />
m<br />
τinel. ,<br />
where τ inel. denotes the lifetime due to inelastic scattering processes. A removal of unwanted<br />
top layers with argon etching and subsequent soft X-ray PES provides access to buried layers,<br />
however, this approach significantly changes the surface morphology and hampers a further<br />
investigation of highly reactive functional layers such as EuO.<br />
Since the last decade, however, the hard X-ray regime (hν 2 keV) has become available to<br />
photoemission – an energy range complementary to the established soft X-rays. This extends<br />
the escape depth of the photoelectrons up to several tens of nanometers according to the estimation<br />
λ ∝ Ekin 0.78,<br />
as depicted in Fig. 2.18.84,85 Thus, HAXPES with photon energies up to<br />
10 keV is perfectly suited to investigate the electronic properties of buried interface or bulk<br />
properties. Hard X-ray excitation, however, implies also drawbacks such as reduced photoemission<br />
cross-sections and Debye-Waller factors, as discussed in Ch. 2.4.3. Fortunately, since<br />
Figure 3.13.: An extra-wide photoemission spectrum by HAXPES. Deep core-levels are accessible and<br />
valence-like levels have reduced cross-sections, as illustrated in a survey spectrum taken at hν =<br />
4 keV. The spectrum of a buried SiO x interface layer (inset) varies in observable SiO x fraction<br />
with excitation energy.