Abstract
We report a comparative study of temperature-dependent photoluminescence and structural dynamics of two perovskite semiconductors, the chalcogenide BaZrS3 and the halide CsPbBr3. These materials have similar crystal structures and direct band gaps, but we find that they have quite distinct optoelectronic and vibrational properties. Both materials exhibit thermally activated nonradiative recombination, but the nonradiative recombination rate in BaZrS3 is four orders of magnitude faster than in CsPbBr3, for the crystals studied here. Raman spectroscopy reveals that the effects of phonon anharmonicity are far more pronounced in CsPbBr3 than in BaZrS3. Further, although both materials feature a large dielectric response due to low-energy polar optical phonons, the phonons in CsPbBr3 are substantially lower in energy than in BaZrS3. Our results suggest that electron-phonon coupling in BaZrS3 is more effective at nonradiative recombination than in CsPbBr3 and that BaZrS3 may also have a substantially higher concentration of nonradiative recombination centers than CsPbBr3. The low defect concentration in CsPbBr3 may be related to the ease of lattice reconfiguration, typified by anharmonic bonding. It remains to be seen to what extent these differences are inherent to the chalcogenide and halide perovskites and to what extent they can be affected by materials processing.
Original language | English |
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Article number | 085402 |
Journal | Physical Review Materials |
Volume | 8 |
Issue number | 8 |
DOIs | |
Publication status | Published - Aug 2024 |
Funding
We acknowledge the support of Dr. I. Pinkas (WIS) for help designing the experimental setup, Dr. L. Segev (WIS) for developing the Raman software, and Dr. S. Aharon (Princeton) for help in the synthesis of CsPbBr3 crystals. O.Y. acknowledges funding from the European Research Council starting grant (850041 - ANHARMONIC). We acknowledge support from the MIT-Israel Zuckerman STEM Fund and the Sagol Weizmann-MIT Bridge Program. We acknowledge support from the United States-Israel Binational Science Foundation, Grant no. 2020270. We acknowledge support from the National Science Foundation (NSF) under Grant No. 1751736. We acknowledge support from the Skolkovo Institute of Science and Technology and the MIT-Skoltech Next Generation Program. K.Y. acknowledges support from the NSF Graduate Research Fellowship, Grant No. 1745302. B.Z. and J.R. acknowledge support from an ARO MURI with Award No. W911NF-21-1-0327, an NSF grant with Award No. DMR-2122071, and an ONR grant with Award No. N00014-23-1-2818. F.K. acknowledges support from the Swedish Research Council (VR) program 2020-04630, and the Swedish e-Science Research Centre (SeRC). The computations were enabled by resources provided by the National Academic Infrastructure for Supercomputing in Sweden (NAISS) at NSC and PDC partially funded by the Swedish Research Council through Grant Agreement No. 2022-06725. Publisher Copyright: © 2024 American Physical Society.
All Science Journal Classification (ASJC) codes
- General Materials Science
- Physics and Astronomy (miscellaneous)