Kesterite solar cells: Germanium promises better opto-electronic properties than tin
Kesterites are semiconductor compounds made of the elements copper, tin, zinc, and selenium. These semiconductors can be used as an optical absorber material in solar cells, but so far have only achieved a maximum efficiency of 12.6 per cent, while solar cells made of copper-indium-gallium-selenide (CIGS) already attain efficiencies of over 20 percent. Nevertheless, kesterites are considered interesting alternatives to CIGS solar cells because they consist of common elements, so that no supply bottlenecks are to be expected. A team led by Professor Susan Schorr at the HZB has now investigated a series of non-stoichiometric kesterite samples and shed light on the relationship between composition and the opto-electronic properties. During the synthesis of the samples at the HZB, the tin atoms were replaced with germanium.
Neutron diffraction at BER II
The researchers then investigated these samples using neutron diffraction at BER II. Copper, zinc, and germanium can be distinguished from each other particularly well with this method, and their positions can be located in the crystal lattice. The result: kesterites with a slightly copper-poor and zinc-rich composition found in solar cells with the highest efficiencies also have the lowest concentration of point defects as well as the lowest disorder of copper-zinc. The more the composition was enriched with copper, the higher the concentration was of other point defects considered to be detrimental to the performance of solar cells. Further investigations showed how the energy band gap, as it is known, depends on the composition of the kesterite powder samples.
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