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掺镱CrX(X = Cl、Br、I)范德华化合物中的发光与共价性

Luminescence and Covalency in Ytterbium-Doped CrX (X = Cl, Br, I) van der Waals Compounds.

作者信息

Snoeren Thom J, Pressler Kimo, Kluherz Kyle T, Walsh Kelly M, De Yoreo James J, Gamelin Daniel R

机构信息

Department of Chemistry, University of Washington, Seattle, Washington 98195, United States.

Physical Sciences Division, Pacific Northwest National Laboratory, Richland, Washington 99352, United States.

出版信息

J Am Chem Soc. 2023 Aug 9;145(31):17427-17434. doi: 10.1021/jacs.3c05989. Epub 2023 Jul 31.

Abstract

The layered 2D van der Waals ferromagnets CrX (X = Cl, Br, I) show broad d-d photoluminescence (PL). Here we report preparation, structural characterization, and spectroscopic studies of all three CrX compounds doped with the optical impurity, Yb. EXAFS measurements show very similar Cr K-edge and Yb L-edge data for each doped compound, and good fits of the latter are obtained for structures having Yb occupying substitutional octahedral sites. Yb-X bond lengths are systematically ∼0.25 Å larger than their Cr-X counterparts. 4 K PL measurements show efficient sensitization of Yb luminescence upon photoexcitation into lattice absorption bands [Cr d-d and ligand-to-metal charge-transfer (LMCT)] for all three compounds, converting their nondescript broadband d-d PL into sharp f-f emission. The PL of CrCl:Yb and CrBr:Yb occurs at energies typical for [YbX] with these halides, with PL decay times of 0.5-1.0 ms at 4 K, but CrI:Yb displays anomalously low-energy Yb emission and an unusually short PL decay time of only 8 μs at 4 K. Data analysis and angular overlap model (AOM) calculations show that Yb in CrI:Yb has a lower spin-orbit splitting energy than reported for any other Yb in any other compound. We attribute these observations to exceptionally high covalency of the Yb f orbitals in CrI:Yb stemming primarily from the shallow valence-shell ionization potentials of the iodide anions.

摘要

层状二维范德华铁磁体CrX(X = Cl、Br、I)呈现出较宽的d-d光致发光(PL)。在此,我们报告了掺杂光学杂质Yb的所有三种CrX化合物的制备、结构表征和光谱研究。扩展X射线吸收精细结构(EXAFS)测量表明,每种掺杂化合物的Cr K边和Yb L边数据非常相似,对于Yb占据替代八面体位置的结构,后者能得到很好的拟合。Yb-X键长系统地比其对应的Cr-X键长大约0.25 Å。4 K下的PL测量表明,对于所有三种化合物,当光激发进入晶格吸收带[Cr d-d和配体-金属电荷转移(LMCT)]时,Yb发光得到有效敏化,将它们无特征的宽带d-d PL转换为尖锐的f-f发射。CrCl:Yb和CrBr:Yb的PL出现在这些卤化物[YbX]的典型能量处,在4 K下PL衰减时间为0.5 - 1.0 ms,但CrI:Yb显示出异常低能量的Yb发射,在4 K下PL衰减时间异常短,仅为8 μs。数据分析和角重叠模型(AOM)计算表明,CrI:Yb中的Yb自旋轨道分裂能比任何其他化合物中的任何其他Yb都要低。我们将这些观察结果归因于CrI:Yb中Yb f轨道的共价性异常高,这主要源于碘阴离子浅的价壳层电离势。

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