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Diploma - Max Planck Institute for Solid State Research

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4.2 Hybridization: localized versus itinerant states 51<br />

the VB yields a more appropriate model [67] (denoted by model 2 “superposition of<br />

localized levels”).<br />

To illustrate this distinction, both models are presented in fig. 4.18. Exemplarily, two<br />

localized levels differing by a factor of two in spectral intensity and a hole-like parabolic<br />

VB with its apex located 0.2 eV above the Fermi level are taken. On the left-hand side<br />

in (a) as well as in (b) the initial configuration is depicted followed by the rearranged<br />

eigenenergy distribution. A sketch of both components in model 2 the sum of which<br />

represents the spectrum, clarifies the degeneracy of the spectral eigenvalues in regions<br />

of the VB separated from the localized levels. The main disparity between both is the<br />

occurance of a band gap in the case of coupled localized levels, which is not present in<br />

case of superposition. Furthermore, due to the constant symmetry parameter C ij also<br />

the localized states in model 1 will be pushed apart if no valence band approaches. A<br />

feasible correction would be to make it proportional to the distance between the valence<br />

band and the second localized level or solving the model self-consistently re-adjusting<br />

the input parameters of the localized levels so the solution fits in the limit of ɛ i → ∞<br />

to the original PE spectrum.<br />

In the following part, the motivated model 2 <strong>for</strong> europium (hence C ij (k) = 0 and<br />

N f = 1) will be evaluated <strong>for</strong> Si and Eu terminated surfaces. As input <strong>for</strong> the subsurface<br />

PE levels the spectrum calculated by Gerken et. al shifted by 0.15 eV is used. In the<br />

case of a Eu terminated surface, the surface 4f emission is chosen proportional to the<br />

subsurface emission adopted in intensity (6x) and energy position (shifted by 1 eV to<br />

higher binding energies) to the experiment. The distribution of V ij (k), the evolution<br />

of which already has been sketched, is given in fig. 4.17. To verify the coupling to the<br />

projected band structure <strong>for</strong> the Si terminated surface, different numbers of bands have<br />

been taken to simulate the transition from a single band to a continuously-projected<br />

band structure. On the one hand, this effect displaces spectral weight to the edges of the<br />

region where the VB is located and on the other hand distributes the residual weight in<br />

the coupled area yielding an almost homogeneous intensity distribution. In fig. 4.19, this<br />

process is indicated <strong>for</strong> the triangularly shaped area A1 next to the linear dispersive state<br />

at Γ. The final spectra <strong>for</strong> Si and Eu terminated surfaces in Γ−X direction are depicted<br />

in fig. 4.20. The main spectral features are well-reproduced <strong>for</strong> both terminations.<br />

Besides, the measured spectrum <strong>for</strong> Si termination evidences additional interaction with<br />

the projected band structure especially in the region marked by 2. Furthermore, there<br />

has to be a some part of the band structure which causes the accumulation of spectral<br />

weight at the tip of the state S1 (1) not evidenced in the calculated spectrum. Because<br />

only f emission is taken into account in the simulation, the weak VB like contribution (3)<br />

is missing. For the Eu terminated surface, the shift of surface 4f emission with respect<br />

to the subsurface emission has been estimated imprecisely, as well as its width. The<br />

latter is probably related to a different multiplet structure, because the potential is no<br />

longer rotationally symmetric as it can be regarded in bulk as a first approximation.

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