Abstract

Recent technical and commercial successes of existing thin film solar cell technologies motivates exploration of next-generation photovoltaic (PV) absorber materials. Of particular scientific interest are compounds like CuSbSe2_2, which do not have the conventional tetrahedral semiconductor bonding. Here, we demonstrate 1.5 μm thick CuSbSe2_2 PV prototypes prepared at 380-410°C by a self-regulated sputtering process using the conventional substrate device architecture. The p-type CuSbSe2_2 absorber has a 1.1 eV optical absorption onset, ~10510^{5} cm−1^{-1} absorption coefficient at 0.3 eV above the onset, and a hole concentration of ~1017^{17} cm−3^{-3}. The promising >3% energy conversion efficiency (Jsc = 20 mA/cm2^2, FF = 0.44, Voc = 0.35 V) in these initial devices is limited by bulk recombination that limits photocurrent, device engineering issues that affect fill factor, and a photovoltage deficit that likely results from the non-ideal CuSbSe2/CdS band offset.

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