Optical absorption edge of organometallic halide perovskites and its implications for solar cell performance
Bjoern Niesen a, Stefaan De Wolf a, Philipp Löper a, Franz-Josef Haug a, Martin Ledinsky a b, Christophe Ballif a c, Jakub Holovsky b, Jun-Ho Yum c, Sylvain Nicolay c, Julien Bailat c, Soo-Jin Moon c
a Institute of Physics, Academy of Sciences of the Czech Republic, v. v. i., Cukrovarnická 10, Prague, 16200
b PV Center, Centre Suisse d’Electronique et de Microtechnique (CSEM), Jacquet Droz 1, 2000 Neuchâtel
International Conference on Hybrid and Organic Photovoltaics
Proceedings of 6th International Conference on Hybrid and Organic Photovoltaics (HOPV14)
Ecublens, Switzerland, 2014 May 11th - 14th
Organizers: Michael Graetzel and Mohammad Nazeeruddin
Poster, Bjoern Niesen, 347
Publication date: 1st March 2014

 

Organometallic halide perovskite-based solar cells have made rapid progress in recent years. Initially, the perovskite material was mostly utilized to replace the dye in mesoscopic dye-sensitized solar cells. In the meanwhile, it has been demonstrated that perovskite absorber layers work efficiently with solid-state hole-transport layers, even when implemented into planar, scaffold-free devices. In 2014, perovskite-based cell efficiencies have surpassed 16% and open-circuit voltages (Voc) of up to 1.13 V have been reached. Such high Voc values are particularly impressive considering the optical bandgap (EG) of ~1.55 eV for CH3NH3PbI3. Quite generally, the bandgap-voltage offset (EG/q)–VOC, where q is the elementary charge, is a useful measure to assess the electronic quality of the absorber in a solar cell. The small (EG/q)–VOC offset for perovskite-based solar cells thus indicates low detrimental recombination losses, including those via deep defects.

Here, we use highly sensitive photothermal deflection spectroscopy and Fourier-transform photocurrent spectroscopy to reveal the origin of the small (EG/q)–VOCoffset of perovskite-based solar cells. For CH3NH3PbI3 layers at room temperature, we find a band edge with a particularly steep absorption tail, translating into a small Urbach energy of 15 meV, and a sub-bandgap optical absorption below the detection limit (i.e. < 1 cm-1). These results do not only confirm the excellent electronic properties of organometallic halide perovskite thin films but also suggest that the high VOCvalues obtained with perovskite-based solar cells indeed originate from a small defect density and the small structural disorder of the perovskite material. Moreover, we compare these findings with several absorber materials commonly used in solar cells and find a general correlation between the Urbach energy and the (EG/q)–VOC offset.

Finally, we show that the absence of sub-bandgap absorption and the high VOC values make organometallic halide perovskites ideally suited as high-bandgap component cells in tandem solar cells.



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