Chalcogenide perovskites (CPs) have recently emerged
as attractive
thermally and chemically stable candidates to overcome the inherent
instability and toxicity issues of the conventional hybrid organic–inorganic
halide perovskites (OIHPs). However, before further progress can be
made in CP thin-film photovoltaic (PV) cells, there is a need to gain
fundamental insights into their bulk, surface, and interfacial properties.
Herein, we employed density functional theory (DFT) calculations to
systematically characterize the bulk (structural, electronic, and
optical), surface (compositions, relative stabilities, crystal morphology,
and work function), and interfacial (energy band alignment) properties
of BaZrS3, one of the most promising members of the CP
family. BaZrS3 is found to exhibit a direct bandgap of
1.74 eV with small photocarrier effective masses, high absorption
coefficient (∼105 cm–1), low reflectivity
(22%), and low refractive index (2.75), all of which are desirable
characteristics for efficient PV applications. Comprehensive analyses
of the structures, compositions, and relative stabilities of the low-Miller-index
surfaces of BaZrS3 revealed that the (010), (100), and
(111) surfaces are the most stable surfaces, which are also largely
expressed in the Wulff-constructed equilibrium crystal morphology
of BaZrS3. Based on the computed ionization potential (IP)
and electron affinity (EA), we have constructed a vacuum-aligned energy
band diagram of BaZrS3 with commonly used hole- and electron-transport
materials (HTMs and ETMs, respectively). CuI (HTM) and CdS (ETM) are
predicted as the best heterojunction materials to form favorable alignment
(staggered type II) with optimum band offsets with the BaZrS3(111) surface for efficient charge-carrier separation and improved
solar cell performance. Our results show great promise for developing
more efficient and stable BaZrS3-based chalcogenide perovskite
solar cells.