Dec 3, 2024
11:00am - 11:15am
Hynes, Level 1, Room 107
Zhenkun Yuan1,Diana Dahliah2,3,Romain Claes2,Andrew Pike1,David Fenning4,Gian-Marco Rignanese2,Geoffroy Hautier1
Dartmouth College1,Université Catholique de Louvain2,An-Najah National University3,University of California, San Diego4
Zhenkun Yuan1,Diana Dahliah2,3,Romain Claes2,Andrew Pike1,David Fenning4,Gian-Marco Rignanese2,Geoffroy Hautier1
Dartmouth College1,Université Catholique de Louvain2,An-Najah National University3,University of California, San Diego4
The chalcogenide perovskite BaZrS<sub>3</sub> has attracted much attention as a promising solar absorber for thin-film photovoltaics. In this talk, we present our first-principles results on carrier transport and defect properties in this material. We find that BaZrS<sub>3</sub> has a phonon-limited electron mobility of 37 cm<sup>2</sup>/Vs comparable to that in halide perovskites but lower hole mobility of 11 cm<sup>2</sup>/Vs. The defect calculations, based on advanced hybrid density functional theory, indicate that BaZrS<sub>3</sub> is intrinsically n-type due to shallow sulfur vacancies, but that strong compensation by sulfur vacancies will prevent attempts to make it p-type. We also establish that BaZrS<sub>3</sub> is a defect-tolerant absorber with few low-formation-energy, deep intrinsic defects. Among the deep defects, sulfur interstitials are the strongest nonradiative recombination centers which in sulfur-rich conditions would limit the carrier lifetime to 10 ns. Our work highlights the material’s intrinsic limitations in carrier mobility and suggests suppressing the formation of sulfur interstitials to reach long carrier lifetime.