22.09.2015 Views

Association

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

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

SHOW MORE
SHOW LESS
  • No tags were found...

You also want an ePaper? Increase the reach of your titles

YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.

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.

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!