Helical magnetic order and Fermi surface nesting in noncentrosymmetric ScFeGe

Sunil K. Karna, D. Tristant, J. K. Hebert, G. Cao, R. Chapai, W. A. Phelan, Q. Zhang, Y. Wu, C. Dhital, Y. Li, H. B. Cao, W. Tian, C. R. Dela Cruz, A. A. Aczel, O. Zaharko, A. Khasanov, M. A. McGuire, A. Roy, W. Xie, D. A. BrowneI. Vekhter, V. Meunier, W. A. Shelton, P. W. Adams, P. T. Sprunger, D. P. Young, R. Jin, J. F. Ditusa

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Abstract

An investigation of the structural, magnetic, thermodynamic, and charge transport properties of noncentrosymmetric hexagonal ScFeGe reveals it to be an anisotropic metal with a transition to a weak itinerant incommensurate helimagnetic state below TN=36 K. Neutron diffraction measurements discovered a temperature and field independent helical wave vector k = (0 0 0.193) with magnetic moments of 0.53 μB per Fe confined to the ab plane. Density functional theory calculations are consistent with these measurements and find several bands that cross the Fermi level along the c axis with a nearly degenerate set of flat bands just above the Fermi energy. The anisotropy found in the electrical transport is reflected in the calculated Fermi surface, which consists of several warped flat sheets along the c axis with two regions of significant nesting, one of which has a wave vector that closely matches that found in the neutron diffraction. The electronic structure calculations, along with a strong anomaly in the c-axis conductivity at TN, signal a Fermi surface driven magnetic transition, similar to that found in spin density wave materials. Magnetic fields applied in the ab plane result in a metamagnetic transition with a threshold field of ≈6.7 T along with a sharp, strongly temperature dependent discontinuity and a change in sign of the magnetoresistance for in-plane currents. Thus, ScFeGe is an ideal system to investigate the effect of in-plane magnetic fields on a helimagnet with a c-axis propagation vector, where the relative strength of the magnetic interactions and anisotropies determine the topology and magnetic structure.

Original languageEnglish
Article number014443
JournalPhysical Review B
Volume103
Issue number1
DOIs
StatePublished - Jan 27 2021

Funding

The experimental material presented here is supported by the US Department of Energy under EPSCoR Grant No. DE-SC0012432 with additional support from the Louisiana Board of Regents. This research used resources at the High Flux Isotope Reactor, a DOE Office of Science User Facility operated by the Oak Ridge National Laboratory. Part of this work was performed at the Swiss Spallation Neutron Source SINQ, Paul Scherrer Institut, Villigen, Switzerland. The computational work conducted by W.A.S. and D.T. was also supported by the US Department of Energy under EPSCoR Grant No. DE-SC0012432 with additional support from the Louisiana Board of Regents. I.V. acknowledges support from NSF Grant No. DMR 1410741 for theoretical work. Part of this work was performed using supercomputing resources provided by the Center for Computation and Technology (CCT) at Louisiana State University and the Center for Computational Innovations (CCI) at Rensselaer Polytechnic Institute.

FundersFunder number
Center for Computation and Technology
Center for Computational Innovations
US Department of Energy
National Science FoundationDMR 1410741
Directorate for Mathematical and Physical Sciences1410741
Office of Experimental Program to Stimulate Competitive ResearchDE-SC0012432
Office of Science
Oak Ridge National Laboratory
Louisiana Board of Regents
Rensselaer Polytechnic Institute
Louisiana State University

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