Through density functional theory
calculations, we show that the
alloy perovskite system BaZr<sub>1–<i>x</i></sub>Ti<sub><i>x</i></sub>S<sub>3</sub> (<i>x</i> <
0.25) is a promising candidate for producing high power conversion
efficiency (PCE) solar cells with ultrathin absorber layers. To maximize
the minority carrier lifetime, which is important for achieving high
PCE, the defect calculations show that BaZr<sub>1–<i>x</i></sub>Ti<sub><i>x</i></sub>S<sub>3</sub> films should be
synthesized under moderate (i.e., near stoichiometric) growth conditions
to minimize the formation of deep-level defects. The perovskite BaZrS<sub>3</sub> is also found to exhibit ambipolar self-doping properties,
indicating the ability to form homo p–n junctions. However,
our theoretical calculations and experimental solid-state reaction
efforts indicate that the doped perovskite BaZr<sub>1–<i>x</i></sub>Ti<sub><i>x</i></sub>S<sub>3</sub> (<i>x</i> > 0) may not be stable under thermal equilibrium growth
conditions. Calculations of decomposition energies suggest that introducing
compressive strain may be a plausible approach to stabilize BaZr<sub>1–<i>x</i></sub>Ti<sub><i>x</i></sub>S<sub>3</sub> thin films