Room Temperature Excitonic Structure in Li-doped CsPbBr3 Nanocrystals Via Two Photon Absorption
ORAL
Abstract
This talk investigates the nonlinear photoluminescence (PL) response of CsPbBr3 nanocrystals (NCs) embedded in a Cs2PbBr6 matrix under 800 nm excitation. X-ray diffraction (XRD) confirms a cubic phase for all samples. Linear absorption spectra for both doping levels yield consistent electronic bandgaps; Li incorporation does not measurably shift the band edge, indicating that Li acts primarily as a passivator of surface and impurity states rather than a lattice substituent.
Across fluences of 0.509 mJ cm−2–20.37 mJ cm−2, the room-temperature PL shows pronounced excitonic structure, departing from the single-Gaussian line shape often reported. At low fluence, log–log fits of peak intensity versus fluence give slopes near 2, consistent with two-photon absorption as the dominant excitation pathway. At higher fluence, we observe spectral narrowing and threshold-like behavior indicative of optical gain/amplified spontaneous emission (ASE), with lower apparent thresholds in Li-doped samples. Together, the unchanged band edge and the PL gain behavior establish a stable, room-temperature platform for nonlinear and gain-enabled photonics.
Across fluences of 0.509 mJ cm−2–20.37 mJ cm−2, the room-temperature PL shows pronounced excitonic structure, departing from the single-Gaussian line shape often reported. At low fluence, log–log fits of peak intensity versus fluence give slopes near 2, consistent with two-photon absorption as the dominant excitation pathway. At higher fluence, we observe spectral narrowing and threshold-like behavior indicative of optical gain/amplified spontaneous emission (ASE), with lower apparent thresholds in Li-doped samples. Together, the unchanged band edge and the PL gain behavior establish a stable, room-temperature platform for nonlinear and gain-enabled photonics.
*Acknowledgment: This material is based upon work supported by the Air Force Office of Scientific Research under award number FA9550-24-1-0059. We also acknowledge the support ofL. C. Hassinger Fellowship. A portion of this work was performed at the National High Magnetic Field Laboratory, which is supported by the National Science Foundation CooperativeAgreement No. DMR-2128556 and the State of Florida.
–
Presenters
-
Parisa Alimohamadi
- University of Florida