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Competing energetic states in γ-Fe<sub>2</sub>WO<sub>6</sub> with strong spin-charge-lattice coupling

ORAL

Abstract

We report magnetic and electronic properties of γ-Fe2WO6 via neutron powder diffraction measurements and first-principles density function theory calculations. We reveal a magnetic ground state which is distinct from an earlier report [1], despite the fact that both materials studied have the same space group but with slightly different atomic positions. Interestingly, both spin structures are well captured by first-principles calculations. Furthermore, we show that the spin structures of this system are correlated with electronic properties, with one being insulating and the other being metallic. These features suggest that γ-Fe2WO6 exhibits competing energetic states in which spin, charge, and lattice degrees of freedom are strongly coupled to each other.

[1] H. Pinto, M. Melamud, and H. Shaked, Acta Crystallogr., Sect. A: Cryst. Phys., Diffr., Theor. Gen. Crystallogr. 33, 663 (1977).

Presenters

  • Milos Sretenovic

    Department of Physics and Astronomy, Michigan State University

Authors

  • Milos Sretenovic

    Department of Physics and Astronomy, Michigan State University

  • Satoshi Okamoto

    Oak Ridge National Lab, Materials Science and Technology Division, Oak Ridge National Laboratory, Oak Ridge National Laboratory

  • Gordon Peiker

    University of California San Diego

  • Xudong Tang

    Department of Physics and Astronomy, Michigan State University

  • Heda Zhang

    Department of Physics and Astronomy, Michigan State University

  • CQ Xu

    Department of Physics and Astronomy, Michigan State University

  • Thomas W Heitmann

    University of Missouri, University of Missouri Research Reactor, The Missouri Research Reactor, University of Missouri, Columbia, Missouri, Missouri Research Reactor, University of Missouri, University of Missouri Research Reactor, University of Missouri

  • Clarina Dela Cruz

    Oak Ridge National Lab, Materials Science and Technology Division, Oak Ridge National Laboratory

  • Xianglin Ke

    Michigan State University, Department of Physics and Astronomy, Michigan State University