Relief of frustration in the Heisenberg pyrochlore antiferromagnet Gd2Pt2O7

The gadolinium pyrochlores Gd2B2O7 are among the best realizations of antiferromagnetically coupled Heisenberg spins on a pyrochlore lattice. We present a magnetic characterization of Gd2Pt2O7, a unique member of this family. Magnetic susceptibility, heat capacity, and muon spin relaxation measureme...

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Bibliographic Details
Published in:Physical review. B 2016-10, Vol.94 (13), p.134417
Main Authors: Hallas, A M, Sharma, A Z, Cai, Y, Munsie, T J, Wilson, M N, Tachibana, M, Wiebe, C R, Luke, G M
Format: Article
Language:English
Subjects:
Antiferromagnetism
Excitation spectra
Frustration
Gadolinium
Magnetic permeability
Magnetic properties
Magnetism
Muon spin relaxation
Platinum
Pyrochlores
Sharpness
Specific heat
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Summary:The gadolinium pyrochlores Gd2B2O7 are among the best realizations of antiferromagnetically coupled Heisenberg spins on a pyrochlore lattice. We present a magnetic characterization of Gd2Pt2O7, a unique member of this family. Magnetic susceptibility, heat capacity, and muon spin relaxation measurements show that Gd2Pt2O7 undergoes an antiferromagnetic ordering transition at TN=1.6 K. This transition is strongly first order, as indicated by the sharpness of the heat capacity anomaly, thermal hysteresis in the magnetic susceptibility, and a nondivergent relaxation rate in μSR. The form of the heat capacity below TN suggests that the ground state is an anisotropic collinear antiferromagnet with an excitation spectrum that is gapped by 0.245(1) meV. The ordering temperature in Gd2Pt2O7,TN=1.6 K, is a substantial 160% increase from other gadolinium pyrochlores, which are all known to order at 1 K or lower. We attribute this enhancement in TN to the B-site cation, platinum. Despite being nonmagnetic, platinum has a filled 5dt2g orbital and an empty 5deg orbital that can facilitate superexchange. Thus, the magnetic frustration in Gd2Pt2O7 is partially “relieved,” thereby promoting magnetic order.
ISSN:2469-9950
2469-9969
DOI:10.1103/PhysRevB.94.134417