Probing the Jeff=0 ground state and the Van Vleck paramagnetism of the Ir5+ ions in the layered Sr2Co0.5Ir0.5O4

We report a combined experimental and theoretical x-ray magnetic circular dichroism (XMCD) spectroscopy study at the Ir-L2,3 edges on the Ir5+ ions of the layered hybrid solid state oxide Sr2Co0.5Ir0.5O4 with the K2NiF4 structure. From theoretical simulation of the experimental Ir-L2,3 XMCD spectrum...

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Bibliographic Details
Main Authors: Agrestini, Stefano (Author) , Haverkort, Maurits W. (Author)
Format: Article (Journal)
Language:English
Published: 29 June 2018
In: Physical review
Year: 2018, Volume: 97, Issue: 21
ISSN:2469-9969
DOI:10.1103/PhysRevB.97.214436
Online Access:Verlag, Volltext: http://dx.doi.org/10.1103/PhysRevB.97.214436
Verlag, Volltext: https://link.aps.org/doi/10.1103/PhysRevB.97.214436
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Author Notes:S. Agrestini, C.-Y. Kuo, K. Chen, Y. Utsumi, D. Mikhailova, A. Rogalev, F. Wilhelm, T. Förster, A. Matsumoto, T. Takayama, H. Takagi, M.W. Haverkort, Z. Hu, and L.H. Tjeng
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Summary:We report a combined experimental and theoretical x-ray magnetic circular dichroism (XMCD) spectroscopy study at the Ir-L2,3 edges on the Ir5+ ions of the layered hybrid solid state oxide Sr2Co0.5Ir0.5O4 with the K2NiF4 structure. From theoretical simulation of the experimental Ir-L2,3 XMCD spectrum, we found a deviation from a pure Jeff=0 ground state with an anisotropic orbital-to-spin moment ratio (Lx/2Sx=0.43 and Lz/2Sz=0.78). This deviation is mainly due to multiplet interactions being not small compared to the cubic crystal field and due to the presence of a large tetragonal crystal field associated with the crystal structure. Nevertheless, our calculations show that the energy gap between the singlet ground state and the triplet excited state is still large and that the magnetic properties of the Ir5+ ions can be well described in terms of singlet Van Vleck paramagnetism.
Item Description:Im Titel sind "eff", "2", "0.5" und "4" tiefgestellt
Im Titel ist "5+" hochgestellt
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Physical Description:Online Resource
ISSN:2469-9969
DOI:10.1103/PhysRevB.97.214436