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Phys. Rev. B 72, 014425 (2005) [16 pages]

Magnetic ordering and effects of crystal electric field anisotropy in the hexagonal compounds RPtIn (R=Y,Gd–Lu)

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E. Morosan, S. L. Bud’ko, and P. C. Canfield
Ames Laboratory and Department of Physics and Astronomy, Iowa State University, Ames, Iowa 50011, USA

Received 3 February 2005; revised 14 April 2005; published 12 July 2005

Single crystals of RPtIn R=Y, Gd–Lu were grown out of In-rich ternary solution. Powder x-ray diffraction data on all of these compounds were consistent with the hexagonal ZrNiAl-type structure (space group P6̅ 2m). The R=Tb and Tm members of the series appear to order antiferromagnetically (TN=46.0 and 3.0 K, respectively), whereas the R=Gd, Dy–Er compounds have at least a ferromagnetic component of the magnetization along the c axis. The magnetic ordering temperatures of all of these systems seem to scale well with the de Gennes factor, whereas the curious switching from ferromagnetic to antiferromagnetic ordering across the series is correlated with a change in anisotropy, such that, in the low-temperature paramagnetic state, χab>χc for the antiferromagnetic compounds and χc>χab for the rest. In order to characterize the magnetic ordering across the RPtIn series, a three-dimensional model of the magnetic moments in Fe2P-type systems was developed, using the three coplanar Ising-like systems model previously introduced for the extremely planar TbPtIn compound: given the orthorhombic point symmetry of the R sites, we assumed the magnetic moments to be confined to six nonplanar easy axes, whose in-plane projections are rotated by 60° with respect to each other. Such a model is consistent with the reduced high-field magnetization values observed for the RPtIn compounds R=Tb–Tm, and qualitatively reproduces the features of the angular dependent magnetization of HoxY1−xPtIn at H=55 kG.

© 2005 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevB.72.014425
DOI:
10.1103/PhysRevB.72.014425
PACS:
75.25.+z, 75.10.−b, 75.30.Gw, 75.30.Kz