Uncovering the Origin of Divergence in the CsM(CrO4)2 (M = La, Pr, Nd, Sm, Eu; Am) Family through Examination of the Chemical Bonding in a Molecular Cluster and by Band Structure Analysis

dc.contributor.author Galley, Shane
dc.contributor.author Arico, Alexandra
dc.contributor.author Lee, Tsung-Han
dc.contributor.author Deng, Xiaoyu
dc.contributor.author Yao, Yong-Xin
dc.contributor.author Sperling, Joseph
dc.contributor.author Proust, Vanessa
dc.contributor.author Storbeck, Julia
dc.contributor.author Dobrosavljevic, Vladimir
dc.contributor.author Neu, Jennifer
dc.contributor.author Siegrist, Theo
dc.contributor.author Baumbach, Ryan
dc.contributor.author Albrecht-Schmitt, Thomas
dc.contributor.author Kaltsoyannis, Nikolas
dc.contributor.author Lanata, Nicola
dc.contributor.department Ames National Laboratory
dc.contributor.department Department of Physics and Astronomy
dc.date 2018-03-23T08:40:18.000
dc.date.accessioned 2020-06-29T23:20:47Z
dc.date.available 2020-06-29T23:20:47Z
dc.date.embargo 2019-01-10
dc.date.issued 2018-02-07
dc.description.abstract <p>A series of f-block chromates, CsM(CrO4)(2) (M = La, Pr, Nd, Sm, Eu; Am), were prepared revealing notable differences between the Am-III derivatives and their lanthanide analogs. While all compounds form similar layered structures, the americium compound exhibits polymorphism and adopts both a structure isomorphous with the early lanthanides as well as one that possesses lower symmetry. Both polymorphs are dark red and possess band gaps that are smaller than the Ln(III) compounds. In order to probe the origin of these differences, the electronic structure of alpha-CsSm(CrO4)(2), alpha-CsEu(CrO4)(2), and alpha-CsAm(CrO4)(2) were studied using both a molecular cluster approach featuring hybrid density functional theory and QTAIM analysis and by the periodic LDA+GA and LDA+DMFT methods. Notably, the covalent contributions to bonding by the f orbitals were found to be more than twice as large in the Al-III chromate than in the Sm-III and Eu-III compounds, and even larger in magnitude than the Am-5f spin orbit splitting in this system. Our analysis indicates also that the Am-O covalency in alpha-CsAm(CrO4)(2) is driven by the degeneracy of the 5f and 2p orbitals, and not by orbital overlap.</p>
dc.identifier archive/lib.dr.iastate.edu/ameslab_manuscripts/131/
dc.identifier.articleid 1128
dc.identifier.contextkey 11826251
dc.identifier.s3bucket isulib-bepress-aws-west
dc.identifier.submissionpath ameslab_manuscripts/131
dc.identifier.uri https://dr.lib.iastate.edu/handle/20.500.12876/7048
dc.language.iso en
dc.relation.ispartofseries IS-J 9595
dc.source.bitstream archive/lib.dr.iastate.edu/ameslab_manuscripts/131/IS_J_9584.pdf|||Fri Jan 14 19:44:34 UTC 2022
dc.subject.disciplines Biological and Chemical Physics
dc.subject.disciplines Chemistry
dc.subject.disciplines Physical Chemistry
dc.subject.keywords actinides
dc.subject.keywords americium
dc.subject.keywords electronic structure
dc.subject.keywords quantum theory of atoms in molecules
dc.subject.keywords band structures of actinides
dc.title Uncovering the Origin of Divergence in the CsM(CrO4)2 (M = La, Pr, Nd, Sm, Eu; Am) Family through Examination of the Chemical Bonding in a Molecular Cluster and by Band Structure Analysis
dc.type article
dc.type.genre article
dspace.entity.type Publication
relation.isOrgUnitOfPublication 25913818-6714-4be5-89a6-f70c8facdf7e
relation.isOrgUnitOfPublication 4a05cd4d-8749-4cff-96b1-32eca381d930
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