2018
DOI: 10.1039/c8nr01109e
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Luminescence and thermal behaviors of free and trapped excitons in cesium lead halide perovskite nanosheets

Abstract: Very recently, all-inorganic perovskite CsPbX3 (X = Cl, Br, I) nanostructures such as nanoparticles, nanoplates, and nanorods have been extensively explored. These CsPbX3 nanostructures exhibit excellent optical properties; however, the photophysics involved is not yet clear. Herein, the emission properties and luminescence mechanism of CsPbBr3 nanosheets (NSs) were investigated using steady-state and time-resolved photoluminescence (PL) spectroscopic techniques. Moreover, two kinds of excitonic emissions (Pea… Show more

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Cited by 156 publications
(140 citation statements)
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“…By fitting the temperature dependent FWHM curve, the S factor was derived as 37.17 and the ℏ ω photon was 17.95 meV. The Huang–Rhys factor of Rb 2 CuBr 3 is much higher than that of most traditional luminescent materials, such as ZnSe, CdSe, and CsPbBr 3 , demonstrating its soft crystal nature and the easy formation of STEs in Rb 2 CuBr 3 . The specific excitation and recombination processes for Rb 2 CuBr 3 are shown in the schematic diagram of Figure f.…”
mentioning
confidence: 96%
“…By fitting the temperature dependent FWHM curve, the S factor was derived as 37.17 and the ℏ ω photon was 17.95 meV. The Huang–Rhys factor of Rb 2 CuBr 3 is much higher than that of most traditional luminescent materials, such as ZnSe, CdSe, and CsPbBr 3 , demonstrating its soft crystal nature and the easy formation of STEs in Rb 2 CuBr 3 . The specific excitation and recombination processes for Rb 2 CuBr 3 are shown in the schematic diagram of Figure f.…”
mentioning
confidence: 96%
“…Namely, the lasing region moves faster than the PL with increasing strain. At room temperature, the 527 nm PL peak can be attributed to the emissions of free excitons with high energy, and the emission wavelength is dominated by bandgap rather than defects related energy levels. Therefore, the underlying mechanisms leading to the shifts of the lasing mode and PL emission are different in nature.…”
mentioning
confidence: 99%
“…At higher ranges for lasing (usually n~10 18 cm -3 for 3D perovskites [18]), the key factor that limits the carrier density under CW excitation originates from the Auger recombination coefficient c. It is also clear that the carrier density within perovskite films is proportional to P at low CW excitation intensities (usually lower than~1 to~1000 mW/cm 2 ). In this region, the radiative recombination type can be identified through the logarithmic slope of the CW power-dependent PL intensity ( Figure 3C), whereas slopes of 1 and 2 refer to excitonic (monomolecular) and free electron-hole (bimolecular) recombination, respectively [37,[53][54][55][56]. However, when P increases, the second-order term (bn 2 ) becomes comparable with the first-order term (an), resulting in the nonlinear relationship between P and n ( Figure 3B).…”
Section: Trends In Chemistrymentioning
confidence: 99%