4.8 Article

Covalency in Americium(III) Hexachloride

期刊

JOURNAL OF THE AMERICAN CHEMICAL SOCIETY
卷 139, 期 25, 页码 8667-8677

出版社

AMER CHEMICAL SOC
DOI: 10.1021/jacs.7b03755

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资金

  1. Heavy Element Chemistry Program at LANL by the Division of Chemical Sciences, Geosciences, and Biosciences, Office of Basic Energy Sciences, U.S. Department of Energy
  2. U.S. Department of Energy
  3. National Nuclear Security Administration of U.S. Department of Energy [DE-AC52-06NA25396]
  4. Glenn T. Seaborg Institute
  5. Director's Postdoctoral Fellowship
  6. LANL Marie Curie Fellowship
  7. U.S. Department of Energy, Office of Science, Office of Workforce Development for Teachers and Scientists, Office of Science Graduate Student Research (SCGSR) program
  8. DOE [DE-AC05-06OR23100]
  9. Chemical Sciences, Geosciences, and Biosciences Division of the Office of Basic Energy Sciences of the Department of Energy [DE-SC0004739]
  10. U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences [DE-AC02-76SF00515]
  11. DOE Office of Biological and Environmental Research
  12. National Institutes of Health, National Institute of General Medical Sciences [P41GMI03393]

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Developing a better understanding of covalency (or orbital mixing) is of fundamental importance. Covalency occupies a central role in directing chemical and physical properties for almost any given compound or material. Hence, the concept of covalency has potential to generate broad and substantial scientific advances, ranging from biological applications to condensed matter physics. Given the importance of orbital mixing combined with the difficultly in measuring covalency, estimating or inferring covalency often leads to fiery debate. Consider the 60-year controversy sparked by Seaborg and co-workers (Diamond, R. M.; Street, K., Jr.; Seaborg, G. T. J. Am. Chem. Soc. 1954, 76, 1461) when it was proposed that covalency from 5f-orbitals contributed to the unique behavior of americium in chloride matrixes. Herein, we describe the use of ligand K-edge X-ray absorption spectroscopy (XAS) and electronic structure calculations to quantify the extent of covalent bonding in arguably one of the most difficult systems to study, the Am-Cl interaction within AmCl63-. We observed both 5f- and 6d-orbital mixing with the Cl-3p orbitals; however, contributions from the 6d-orbitals were more substantial. Comparisons with the isoelectronic EuCl63- indicated that the amount of Cl 3p-mixing with Eu-III Sd-orbitals was similar to that observed with the Am-III 6d-orbitals. Meanwhile, the results confirmed Seaborg's 1954 hypothesis that Am-III 5f-orbital covalency was more substantial than 4f-orbital mixing for Eu-III.

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