2001
DOI: 10.1143/jpsj.70.3751
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Amorphous CsPbX3versus Crystalline Cs4PbX6(X=Br, Cl)–Their Localized Electronic States Studied by Optical Absorption Spectroscopy

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Cited by 10 publications
(5 citation statements)
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“…The consideration was recently confirmed by our subsequent measurement 7) of the fundamental absorption spectrum of (crystalline) Cs 4 PbBr 6 , whose crystal structure is composed of a hexagonal regular array of Pb 2þ (Br À ) 6 octahedra with the central Pb 2þ ions mutually isolated by intervening (between the octahedra) Cs þ ions, and whose low-energy absorption characteristics were very similar in feature to those of the amorphous CsPbBr 3 . Despite the close resemblance of the absorption properties between the amorphous CsPbBr 3 and crystalline Cs 4 PbBr 6 , however, they show quite different luminescence properties from each other.…”
Section: Resultsmentioning
confidence: 54%
“…The consideration was recently confirmed by our subsequent measurement 7) of the fundamental absorption spectrum of (crystalline) Cs 4 PbBr 6 , whose crystal structure is composed of a hexagonal regular array of Pb 2þ (Br À ) 6 octahedra with the central Pb 2þ ions mutually isolated by intervening (between the octahedra) Cs þ ions, and whose low-energy absorption characteristics were very similar in feature to those of the amorphous CsPbBr 3 . Despite the close resemblance of the absorption properties between the amorphous CsPbBr 3 and crystalline Cs 4 PbBr 6 , however, they show quite different luminescence properties from each other.…”
Section: Resultsmentioning
confidence: 54%
“…Recently, all-inorganic cesium lead halide perovskites without any organic components have emerged as promising candidates for absorbing layers in solar cells. A CsPbX 3 perovskite, such as CsPbI 3 , exhibits better thermal stability than the OHP . The cubic-structured CsPbI 3 (α-CsPbI 3 phase) has an appropriate band gap (1.73 eV) for solar cell applications .…”
Section: Introductionmentioning
confidence: 99%
“…The correlation between the PL and the absorption spectra indicates that only the CPB113 phase is responsible for the light emission around 520 nm, which originates from the excitonic recombination near the edges of the direct bandgap. ,, The CPB416 phase, alternatively, exhibits a bandgap at a UV wavelength (316 nm) and does not produce PL in the visible range (Figure S1). For verification purposes, we deposited excessive CsBr precursor during the evaporation, which turns out necessary to eliminate trace amount of CPB113 . The thin film obtained in this manner (Sample F) exhibits the negligible PL intensity and the minimal absorbance in the visible range.…”
mentioning
confidence: 99%