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Institute
In this thesis, thin-film solar cells on the basis of Cu(In,Ga)(S,Se)2 (CIGSSe) were investigated.
Until today, most high efficient CIGSSe-based solar cells use a toxic and wetchemical deposited CdS buffer layer, which doesn’t allow a dry inline production. However, a promising and well-performing alternative buffer layer, namely indium sulfide, has been found which doesn’t comprise these disadvantages. In order to shed light on these well-performing devices, the surfaces and in particular the interfaces which play a major role for the charge carrier transport are investigated in the framework of this thesis. Both, the chemical and electronic properties of the solar cells’ interfaces were characterized.
In case of the physical vapor deposition of an InxSy-based buffer layer, the cleaning step of the CdS chemical-bath deposition is not present and thus changes of the absorber surface have to be taken into account. Therefore, adsorbate formation, oxidation, and segregation of absorber elements in dependence of the storing temperature and the humidity are investigated in the first part of this thesis.
The efficiencies of CIGSSe-based solar cells with an InxSy buffer layer depend on the nominal indium concentration x and display a maximum for x = 42 %. In this thesis, InxSy samples with a nominal indium concentration of 40.2% ≤ x ≤ 43.2% were investigated by surface-sensitive and surface-near bulk-sensitive techniques, namely with photoemission spectroscopy (PES) and x-ray emission spectroscopy (XES). The surfaces of the films were found to be sulfur-poor and indium-rich in comparison with stoichiometric In2S3. Moreover, a direct determination of the band alignment at the InxSy/CISSe interface in dependence of the nominal indium concentration x was conducted with the help of PES and inverse PES (IPES) and a flat band alignment was found for x = 42 %.
In order to study the impact of a heat treatment as it occurs during subsequent cell process steps, the indium sulfide-buffered absorbers were annealed for 30 minutes under UHV conditions at 200 °C after the initial data set was taken. Besides a reported enhanced solar cell performance, a significant copper diffusion from the absorber into the buffer layer takes place due to the thermal treatment. Accordingly, the impact of the copper diffusion on the hidden InxSy/CISSe interface was discussed and for x = 40.2% a significant cliff (downwards step in the conduction band) is observed. For increasing x, the alignment in the conduction band turns into a small upwards step (spike) for the region 41% ≤ x ≤ 43.2%. This explains the optimal solar cell performance for this indium contents.
In a further step, the sodium-doped indium sulfide buffer which leads to significantly higher efficient solar cells was investigated. It was demonstrated by PES/IPES that the enhanced performance can be ascribed to a significant larger surface band gap in comparison with undoped InxSy. The occurring spike in the Na:InxSy/CISSe band alignment gets reduced due to a Se diffusion induced by the thermal treatment. Furthermore, after the thermal treatment the sodium doped indium sulfide layer experiences a copper diffusion which is reduced by more than a factor of two compared to pure InxSy.
Next, the interface between the Na:InxSy buffer layer and the i-ZnO (i = intrinsic, non-deliberately doped), as a part of the transparent front contact was analyzed. The i-ZnO/Na:InxSy interface shows significant interdiffusion, leading to the formation of, e.g., ZnS and hence to a reduction of the nominal cliff in the conduction band alignment.
In the last part of this thesis, the well-established surface-sensitive reflective electron energy loss spectroscopy (REELS) was utilized to study the CIGSSe absorber, the InxSy buffer, and annealed InxSy buffer surfaces. By fitting the characteristic inelastic scattering cross sections λK(E) with Drude-Lindhard oscillators the dielectric function was identified. The determined dielectric functions are in good agreement with values from bulk-sensitive optical measurements on indium sulfide layers. In contrast, for the chalcopyrite-based absorber significant differences appear. In particular, a substantial larger surface band gap of the CIGSSe surface of E^Ex_Gap = (1.4±0.2) eV in comparison with bulk values is determined. This provides for the first time an independent verification of earlier PES/IPES results. Finally, the electrons’ inelastic mean free paths l for the three investigated surfaces are compared for different primary energies with theoretical values and the universal curve.
Transition metal oxides (TMO) represent a highly interesting material class as
they exhibit a variety of different emergent phenomena including multiferroicity and
superconductivity. These effects result from a significant interplay of charge, spin
and orbital degrees of freedom within the correlated d-electrons. Oxygen vacancies
(OV) at the surface of certain d0 TMO release free charge carriers and prompt the
formation of a two-dimensional electron gas (2DEG). Barium titanate (BaTiO3) is a
prototypical and promising d0 TMO. It displays ferroelectricity at room temperature
and features several structural phase transitions, from cubic over tetragonal (at
room temperature) and orthorhombic to rhombohedral. The spontaneous electric
polarization in BaTiO3 can be used to manipulate the physical properties of adjacent
materials, e.g. in thin films. Although the macroscopic properties of BaTiO3 are studied
in great detail, the microscopic electronic structure at the surface and interface of
BaTiO3 is not sufficiently understood yet due to the complex interplay of correlation
within the d states, oxygen vacancies at the surface, ferroelectricity in the bulk and
the structural phase transitions in BaTiO3.
This thesis investigates the electronic structure of different BaTiO3 systems by
means of angle-resolved photoelectron spectroscopy (ARPES). The valence band of
BaTiO3 single crystals is systematically characterized and compared to theoretical
band structure calculations. A finite p-d hybridization of titanium and oxygen states
was inferred at the high binding energy side of the valence band. In BaTiO3 thin films,
the occurrence of spectral weight near the Fermi level could be linked to a certain
amount of OV at the surface which effectively dopes the host system. By a systematic
study of the metallic surface states as a function of temperature and partial oxygen
pressure, a model was established which reflects the depletion and accumulation of
charge carriers at the surface of BaTiO3. An instability at T ~ 285K assumes a volatile
behavior of these surface states.
The ferroelectricity in BaTiO3 allows a control of the electronic structure at the interface
of BaTiO3-based heterostructures. Therefore, the interface electronic structure
of Bi/BaTiO3 was studied with respect to the strongly spin-orit coupled states in Bi by
also including a thickness dependent characterization. The ARPES results, indeed,
confirm the presence of Rashba spin-split electronic states in the bulk band gap of the ferroelectric substrate. By varying the film thickness in Bi/BaTiO3, it was able to modify
the energy position and the Fermi vector of the spin-split states. This observation
is associated with the appearance of an interface state which was observed for very
low film thickness. Both spectral findings suggest a significant coupling between the
Bi films and BaTiO3.