Crystal growth and magnetic structure of ternary silicide EuPd3Si2

Shivani Sharma, Masoud Mardani, Keke Feng, Kaya Wei, Ryan Baumbach, Qiang Zhang, David J. Singh, Theo Siegrist

Research output: Contribution to journalArticlepeer-review

1 Scopus citations

Abstract

The hexagonal CaCu5-type structure (P6/mmm) is the prototype for more than 100 ternary borides, gallides, and silicides, with general stoichiometry of RTM3X2 (R=lanthanide/alkalineearth;TM=transitionmetal;X=B,Ga,Si,Ge). We report the synthesis, crystal structure, and bulk magnetic properties of polycrystalline and single crystal samples of EuPd3Si2 and its nonmagnetic analog SrPd3Si2. Both compounds crystallize in the orthorhombic space group symmetry Imma (no. 74, Z=2, oI12) displaying pseudohexagonal symmetry. Ferromagnetic (FM) order of Eu2+ at TC1=78K and a spin-reorientation transition at TC2=5K appear as distinctive features in bulk magnetization, specific heat, and resistivity/resistance measurements. Neutron powder diffraction measurements on EuPd3Si2 confirm FM order of the Eu2+ spins below TC1, with the spins aligned along the a axis below TC2. Electronic band structure calculations corroborate the crystal structure and the FM state for EuPd3Si2, with a Pd d-band polarization in the same direction as the Eu 4f polarization, enhancing the observed spin moment.

Original languageEnglish
Article number023402
JournalPhysical Review Materials
Volume7
Issue number2
DOIs
StatePublished - Feb 2023

Funding

This work is supported by NSF Grant No. DMR-1625780. Part of the work was carried out at the National High Magnetic Field Laboratory, which is supported by NSF Grant No. DMR-1644779 and the State of Florida. Theoretical work at the University of Missouri was supported by the U.S. Department of Energy, Basic Energy Science, Grant No. DE-SC0019114. R.B. was supported by NSF Grant No. DMR-1904361. The research at the Spallation Neutron Source at Oak Ridge National Laboratory was sponsored by the Scientific User Facilities Division, Office of Basic Energy Sciences, U.S. Department of Energy.

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