Bulk electronic structure of non-centrosymmetric EuTGe3 (T=Co, Ni, Rh, Ir) studied by hard x-ray photoelectron spectroscopy

Yuki Utsumi, Deepa Kasinathan, Przemysław Swatek, Oleksandr Bednarchuk, Dariusz Kaczorowski, James M. Ablett, Jean Pascal Rueff

Research output: Contribution to journalArticlepeer-review

Abstract

Non-centrosymmetric EuTGe3 (T= Co, Ni, Rh, and Ir) possesses magnetic Eu2+ ions, and antiferromagnetic ordering appears at low temperatures. Transition-metal substitution leads to changes in the unit-cell volume and in the magnetic ordering. However, the magnetic ordering temperature does not scale with the volume change, and the Eu valence is expected to remain divalent. Here we study the bulk electronic structure of non-centrosymmetric EuTGe3 (T= Co, Ni, Rh, and Ir) by hard x-ray photoelectron spectroscopy. The Eu 3d core-level spectrum confirms the robust Eu2+ valence state against the transition-metal substitution with a small contribution from Eu3+. The estimated Eu mean valence is around 2.1 in these compounds, as confirmed by multiplet calculations. In contrast, the Ge 2p spectrum shifts to higher binding energy upon changing the transition metal from 3d to 4d to 5d elements, hinting at a change in the Ge-T bonding strength. The valence bands of the different compounds are found to be well reproduced by ab initio band structure calculations.

Original languageEnglish (US)
Article number115155
JournalPhysical Review B
Volume97
Issue number11
DOIs
StatePublished - Mar 26 2018
Externally publishedYes

Bibliographical note

Funding Information:
We would like to thank D. Céolin and D. Prieur for their skillful technical assistance. Y.U. thanks K. Mimura and A. Tanaka for helpful discussions. P.S.'s work at Ames Laboratory was supported by the US Department of Energy, Office of Science, Basic Energy Sciences, Materials Science and Engineering Division. Ames Laboratory is operated for the US Department of Energy by Iowa State University under Contract No. DE-AC02-07CH11358. D.K. thanks U. Nitzsche for technical assistance.

Publisher Copyright:
© 2018 American Physical Society.

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