Structural and magnetic properties of two branches of the tripod-kagome-lattice family A2R3Sb3O14 (A = Mg, Zn; R = Pr, Nd, Gd, Tb, Dy, Ho, Er, Yb)

Z. L. Dun, J. Trinh, M. Lee, E. S. Choi, K. Li, Y. F. Hu, Y. X. Wang, N. Blanc, A. P. Ramirez, and H. D. Zhou
Phys. Rev. B 95, 104439 – Published 30 March 2017

Abstract

We present a systematic study of the structural and magnetic properties of two branches of the rare-earth tripod-kagome-lattice (TKL) family A2R3Sb3O14 (A= Mg, Zn; R= Pr, Nd, Gd, Tb, Dy, Ho, Er, Yb; here, we use abbreviation A-R, as in MgPr for Mg2Pr3Sb3O14), which complements our previously reported work on MgDy, MgGd, and MgEr [Z. L. Dun et al., Phys. Rev. Lett. 116, 157201 (2016)]. The present susceptibility (χdc, χac) and specific-heat measurements reveal various magnetic ground states, including the nonmagnetic singlet state for MgPr, ZnPr; long-range orderings (LROs) for MgGd, ZnGd, MgNd, ZnNd, and MgYb; a long-range magnetic charge ordered state for MgDy, ZnDy, and potentially for MgHo; possible spin-glass states for ZnEr, ZnHo; the absence of spin ordering down to 80 mK for MgEr, MgTb, ZnTb, and ZnYb compounds. The ground states observed here bear both similarities as well as striking differences from the states found in the parent pyrochlore systems. In particular, while the TKLs display a greater tendency towards LRO, the lack of LRO in MgHo, MgTb, and ZnTb can be viewed from the standpoint of a balance among spin-spin interactions, anisotropies, and non-Kramers nature of single-ion state. While substituting Zn for Mg changes the chemical pressure, and subtly modifies the interaction energies for compounds with larger R ions, this substitution introduces structural disorder and modifies the ground states for compounds with smaller R ions (Ho, Er, Yb).

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  • Received 27 October 2016
  • Revised 9 February 2017

DOI:https://doi.org/10.1103/PhysRevB.95.104439

©2017 American Physical Society

Physics Subject Headings (PhySH)

Condensed Matter, Materials & Applied Physics

Authors & Affiliations

Z. L. Dun1, J. Trinh2, M. Lee3,4, E. S. Choi4, K. Li5,6, Y. F. Hu5, Y. X. Wang5, N. Blanc2, A. P. Ramirez2, and H. D. Zhou1,4

  • 1Department of Physics and Astronomy, University of Tennessee, Knoxville, Tennessee 37996-1200, USA
  • 2Department of Physics, University of California, Santa Cruz, California 95064, USA
  • 3Department of Physics, Florida State University, Tallahassee, Florida 32306-3016, USA
  • 4National High Magnetic Field Laboratory, Florida State University, Tallahassee, Florida 32310-3706, USA
  • 5Beijing National Laboratory for Molecular Sciences, State Key Laboratory of Rare Earth Materials Chemistry and Applications, College of Chemistry and Molecular Engineering, Peking University, Beijing 100871, People's Republic of China
  • 6Center for High Pressure Science and Technology Advanced Research, Beijing, 100094, People's Republic of China

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Issue

Vol. 95, Iss. 10 — 1 March 2017

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