2020
DOI: 10.1002/ange.202005643
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Room‐Temperature Formation Pathway for CdTeSe Alloy Magic‐Size Clusters

Abstract: Little is known about the pathway of room‐temperature formation of ternary CdTeSe magic‐size clusters (MSCs) obtained by mixing binary CdTe and CdSe induction period samples containing binary precursor compounds (PCs) of MSCs, monomers (Ms), and fragments (Fs). Also, unestablished are dispersion effects that occur when as‐mixed samples (without incubation) are placed in toluene (Tol) and octylamine (OTA) mixtures. The resulting ternary MSCs, exhibiting a sharp optical absorption peak at 399 nm, are labelled Cd… Show more

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Cited by 6 publications
(2 citation statements)
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“…An in situ examination by optical absorption spectroscopy becomes more practical when a reaction proceeds at low temperatures (such as 80 °C or lower) [4, 16, 28–34] . Such a real‐time observation can be essentially continuous, providing a significantly more complete picture of the MSC evolution and transformation.…”
Section: Introductionmentioning
confidence: 99%
See 1 more Smart Citation
“…An in situ examination by optical absorption spectroscopy becomes more practical when a reaction proceeds at low temperatures (such as 80 °C or lower) [4, 16, 28–34] . Such a real‐time observation can be essentially continuous, providing a significantly more complete picture of the MSC evolution and transformation.…”
Section: Introductionmentioning
confidence: 99%
“…Meanwhile, the MSCs can evolve from unique precursor compounds (PCs) via a quasi‐isomerization [1, 4, 24–35] . The PCs are relatively optically transparent at the peak positions of their counterpart MSCs and to longer wavelengths.…”
Section: Introductionmentioning
confidence: 99%