Competing magnetic phases and itinerant magnetic frustration in SrCo2As2

Bing Li, B. G. Ueland, W. T. Jayasekara, D. L. Abernathy, N. S. Sangeetha, D. C. Johnston, Qing-Ping Ding, Y. Furukawa, P. P. Orth, A. Kreyssig, A. I. Goldman, and R. J. McQueeney
Phys. Rev. B 100, 054411 – Published 9 August 2019

Abstract

Whereas magnetic frustration is typically associated with local-moment magnets in special geometric arrangements, here we show that SrCo2As2 is a candidate for frustrated itinerant magnetism. Using inelastic neutron scattering (INS), we find that antiferromagnetic (AF) spin fluctuations develop in the square Co layers of SrCo2As2 below T100 K centered at the stripe-type AF propagation vector of (12,12), and that their development is concomitant with a suppression of the uniform magnetic susceptibility determined via magnetization measurements. We interpret this switch in spectral weight as signaling a temperature-induced crossover from an instability toward ferromagnetism ordering to an instability toward stripe-type AF ordering on cooling, and show results from Monte-Carlo simulations for a J1J2 Heisenberg model that illustrates how the crossover develops as a function of the frustration ratio J1/(2J2). By putting our INS data on an absolute scale, we quantitatively compare them and our magnetization data to exact-diagonalization calculations for the J1J2 model [N. Shannon et al., Eur. Phys. J. B 38, 599 (2004).], and show that the calculations predict a lower level of magnetic frustration than indicated by experiment. We trace this discrepancy to the large energy scale of the fluctuations (Javg75 meV), which, in addition to the steep dispersion, is more characteristic of itinerant magnetism.

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  • Received 23 October 2018
  • Revised 19 June 2019

DOI:https://doi.org/10.1103/PhysRevB.100.054411

©2019 American Physical Society

Physics Subject Headings (PhySH)

Condensed Matter, Materials & Applied Physics

Authors & Affiliations

Bing Li1,2, B. G. Ueland1, W. T. Jayasekara1,2, D. L. Abernathy3, N. S. Sangeetha1, D. C. Johnston1,2, Qing-Ping Ding1,2, Y. Furukawa1,2, P. P. Orth1,2, A. Kreyssig1,2, A. I. Goldman1,2, and R. J. McQueeney1,2

  • 1Ames Laboratory, Ames, Iowa 50011, USA
  • 2Department of Physics and Astronomy, Iowa State University, Ames, Iowa 50011, USA
  • 3Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, USA

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Issue

Vol. 100, Iss. 5 — 1 August 2019

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