A Star-Shaped Heteronuclear (CrMn3II)-Mn-III Species and Its Precise Electronic and Magnetic Structure: Spin Frustration Studied by X-Ray Spectroscopic, Magnetic, and Theoretical Methods

DC FieldValueLanguage
dc.contributor.authorPrinz, Manuel
dc.contributor.authorKuepper, Karsten
dc.contributor.authorTaubitz, Christian
dc.contributor.authorRaekers, Michael
dc.contributor.authorKhanra, Sumit
dc.contributor.authorBiswas, Biplab
dc.contributor.authorWeyhermueller, Thomas
dc.contributor.authorUhlarz, Marc
dc.contributor.authorWosnitza, Joachim
dc.contributor.authorSchnack, Juergen
dc.contributor.authorPostnikov, Andrei V.
dc.contributor.authorSchroeder, Christian
dc.contributor.authorGeorge, Simon J.
dc.contributor.authorNeumann, Manfred
dc.contributor.authorChaudhuri, Phalguni
dc.date.accessioned2021-12-23T16:23:45Z-
dc.date.available2021-12-23T16:23:45Z-
dc.date.issued2010
dc.identifier.issn00201669
dc.identifier.urihttps://osnascholar.ub.uni-osnabrueck.de/handle/unios/14651-
dc.description.abstractMolecular magnets incorporate transition-metal ions with organic groups providing a bridge to mediate magnetic exchange interactions between the ions. Among them are star-shaped molecules in which antiferromagnetic couplings between the central and peripheral atoms are predominantly present. Those configurations lead to an appreciable spin moment in the nonfrustrated ground state. In spite of its topologically simple magnetic structure, the [(CrMn3II)-Mn-III(PyA)(6)Cl-3] (CrMn3) molecule, in which PyA represents the monoanion of syn-pyridine-2-aldoxime, exhibits nontrivial magnetic properties, which emerge from the combined action of single-ion anisotropy and frustration. In the present work, we elucidate the underlying electronic and magnetic properties of the heteronuclear, spin-frustrated CrMn3 molecule by applying X-ray magnetic circular dichroism (XMCD), as well as magnetization measurements in high magnetic fields, density functional theory, and ligand-field multiplet calculations. Quantum-model calculations based on a Heisenberg Hamiltonian augmented with local anisotropic terms enable us not only to improve the accuracy of the exchange interactions but also to determine the dominant local anisotropies. A discussion of the various spin Hamiltonian parameters not only leads to a validation of our element selective transition metal L edge XMCD spin moments at a magnetic field of 5 T and a temperature of 5 K but also allows us to monitor an interesting effect of anisotropy and frustration of the manganese and chromium ions.
dc.description.sponsorshipGraduate College; U.S. Department of EnergyUnited States Department of Energy (DOE) [DE-AC03-76SF00098]; German Research Council (DFG)German Research Foundation (DFG) [FOR 945]; E. Arenholz and J. D. Denlinger are acknowledged for excellent technical support. We would like to thank Joris van Slageren for discussing anisotropy issues with us and for drawing our attention to recent publications on Mn(II) anisotropies. Financial support by the Graduate College and the PhD program (Lower Saxony) is gratefully acknowledged. A.V.P. acknowledges the use of computing resources of the PMMS of the Paul Verlaine University. Part of the work was performed at the Advanced Light Source (A.L.S.), which is supported by the U.S. Department of Energy under Contract No. DE-AC03-76SF00098.; Financial Support from the German Research Council (DFG) in the priority program ``Molecular Magnetism'' as well as through the research group FOR 945 is also thankfully acknowledged.
dc.language.isoen
dc.publisherAMER CHEMICAL SOC
dc.relation.ispartofINORGANIC CHEMISTRY
dc.subjectABSORPTION
dc.subjectANISOTROPY
dc.subjectChemistry
dc.subjectChemistry, Inorganic & Nuclear
dc.subjectCIRCULAR-DICHROISM
dc.subjectCOMPLEX
dc.subjectION
dc.subjectMN
dc.subjectPROBE
dc.subjectSINGLE-MOLECULE MAGNETS
dc.titleA Star-Shaped Heteronuclear (CrMn3II)-Mn-III Species and Its Precise Electronic and Magnetic Structure: Spin Frustration Studied by X-Ray Spectroscopic, Magnetic, and Theoretical Methods
dc.typejournal article
dc.identifier.doi10.1021/ic9012119
dc.identifier.isiISI:000274626200014
dc.description.volume49
dc.description.issue5
dc.description.startpage2093
dc.description.endpage2102
dc.contributor.orcid0000-0002-6391-6548
dc.contributor.orcid0000-0003-0702-2723
dc.contributor.orcid0000-0002-0399-7999
dc.contributor.orcid0000-0002-4864-5479
dc.contributor.researcheridAAC-5007-2019
dc.contributor.researcheridA-4079-2008
dc.contributor.researcheridG-1397-2016
dc.contributor.researcheridG-6730-2012
dc.identifier.eissn1520510X
dc.publisher.place1155 16TH ST, NW, WASHINGTON, DC 20036 USA
dcterms.isPartOf.abbreviationInorg. Chem.
crisitem.author.deptFB 04 - Physik-
crisitem.author.deptFB 04 - Physik-
crisitem.author.deptidfb04-
crisitem.author.deptidfb04-
crisitem.author.orcid0000-0003-0702-2723-
crisitem.author.parentorgUniversität Osnabrück-
crisitem.author.parentorgUniversität Osnabrück-
crisitem.author.netidKuKa120-
crisitem.author.netidScJu137-
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