Apr 25, 2024
4:30pm - 4:45pm
Room 334, Level 3, Summit
Kyle Sendgikoski1,Brendon Jones2,Michael Stewart1,Barbara Marcheschi1,Todd Brintlinger1,John Lyons1,Sarah Brittman1
U. S. Naval Research Laboratory1,Florida State University2
Kyle Sendgikoski1,Brendon Jones2,Michael Stewart1,Barbara Marcheschi1,Todd Brintlinger1,John Lyons1,Sarah Brittman1
U. S. Naval Research Laboratory1,Florida State University2
Halide perovskites have already demonstrated impressive optoelectronic performance in applications ranging from photovoltaics, to light-emitting diodes and lasers, to X-ray and gamma-ray detectors and scintillators. Understanding how extrinsic dopants behave in this class of materials is a critical next step to gaining greater control over the stability and performance of this versatile class of materials.<br/><br/>While Bi<sup>3+</sup> was originally proposed as a potential n-type dopant in lead halide perovskites, experiments and theory clearly demonstrate that it is a deep-level trap that gives rise to broad near-infrared emission. We synthesized a series of crystals of CsPbBr<sub>3</sub> doped with Bi content ranging from 0.01 to 0.32 atomic percent, as quantified by inductively coupled plasma optical emission spectroscopy (ICP-OES). The absorption edge shifts redder with Bi incorporation, but density function theory (DFT) calculations show that this increased absorption comes from the electronic structure of Bi as a deep-level trap, not from a shift in the CsPbBr<sub>3</sub> band edge. Indeed, all doped crystals emit both narrow band-edge (2.37 eV) and broad defect-level (1.12 eV) photoluminescence at room temperature, consistent with our theoretical prediction. We also apply STEM-EDS to the most heavily doped samples to characterize the spatial uniformity of the Bi incorporation within the CsPbBr<sub>3</sub> crystals. Our combined results demonstrate the power of current theoretical approaches to predict defect behavior in halide perovskites, which will be invaluable in guiding the development of these materials.