Abstract
Recent progress in the power conversion efficiency of $\mathrm{Cu}(\mathrm{In},\mathrm{Ga})\mathrm{S}{\mathrm{e}}_{2}$ thin film solar cells has been achieved by an alkali postdeposition treatment. This treatment has been shown to change the surface composition and structure as well as the bulk properties. To investigate the relative importance of those two effects we study the impact of the treatment on Cu-rich and Cu-poor $\mathrm{CuInS}{\mathrm{e}}_{2}$, which show a different influence of interface recombination without the treatment. We develop a potassium postdeposition treatment that can be applied to Cu-rich material, where an additional etching step is necessary. The same postdeposition treatment with etching step is applied to Cu-poor material. In both cases we observe an increase of the power conversion efficiency and open circuit voltage. Comparing the increase in open circuit voltage to the increase in quasi-Fermi level splitting indicates that the improvement in Cu-poor solar cells is mostly due to changes in the bulk, whereas in Cu-rich solar cells both the bulk and the interface are improved. The improvement of the interface is corroborated by temperature dependent current-voltage characteristics, which show that the dominating recombination path in Cu-rich solar cells moves from the interface to the bulk after treatment and by admittance spectroscopy, which shows that the treatment removes a 200 meV deep defect. Photoluminescence spectroscopy shows that even in Cu-rich material the alkali treatment creates a Cu-poor surface, which in this case cannot be created by diffusion of Cu into the bulk, but is grown during the treatment.
Highlights
Copper indium gallium di-selenide, Cu(In, Ga)Se2 or CIGS, represents the most efficient absorber for thin film solar cells, reaching power conversion efficiencies (PCE) up to 22.9% on the laboratory scale [1,2]
The ternary compound copper indium di-selenide (CIS) is less complex compared to CIGS, making it a good material to study the manifold effects of a KF postdeposition treatment (PDT)
We use the fundamental differences in the dominating recombination path between Cu-rich and Cu-poor CuInSe2 to study the effects of the alkali postdeposition treatment
Summary
Copper indium gallium di-selenide, Cu(In, Ga)Se2 or CIGS, represents the most efficient absorber for thin film solar cells, reaching power conversion efficiencies (PCE) up to 22.9% on the laboratory scale [1,2]. The ternary compound copper indium di-selenide (CIS) is less complex compared to CIGS, making it a good material to study the manifold effects of a KF PDT. CuInSe2 and Cu(In, Ga)Se2 can be grown under Cu-poor or Cu-rich conditions that result in very different semiconductor properties. Solar cells are generally made of Cu-poor material, since it results in better PCEs [5]. In the past we have demonstrated, that the semiconductor properties of absorbers grown under Cu-excess are favorable compared to Cu-poor ones [5]: less compensation, lower defect densities, no electrostatic potential fluctuations, higher mobilities, and larger grains. It has long been known that the absorbers grown under Cu-excess exhibit problematic surface
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