Chalcopyrite or chalcopyrite ore (chalcopyrite) are commonly occurring minerals and I–III–VI2 compounds that contain copper, additional metals such as indium and gallium, as well as sulfur and selenium. Many chalcopyrites absorb light very well, exhibit semiconducting properties, and are therefore well suited for manufacturing thin-film solar cells. By varying the chemical composition of the individual elements, the semiconductor properties such as lattice constant and band gap can be adjusted. These are excellent prerequisites for optimizing solar cells.
A chalcopyrite or CIGS thin-film solar cell consists of multiple layers. A glass carrier is commonly used as the substrate. A non-transparent molybdenum layer is applied as the back contact. To form the chalcopyrite layer, copper, indium and gallium are first deposited on the substrate. Subsequently, this layer is selenized or sulfurized in a furnace or an RTP system at temperatures around 550 °C. Hydrogen selenide H2Se or hydrogen sulfide H2S serve as selenium or sulfur sources.
On top of this CIGS layer, which is also referred to as the absorber, a thin cadmium sulfide CdS layer is deposited, followed by a transparent conductive oxide (TCO) that serves as the front contact, for example zinc oxide ZnO. At the interface between the CdS and CIGS layers, charge carrier generation occurs when exposed to sunlight.
Constructing the CIGS solar cell in reverse order, i.e. with the glass substrate on the front side, is also fundamentally possible. This configuration is called the superstrate configuration, because the carrier sits above the cell rather than below it as in the previously described substrate configuration.
