Order by virtual crystal field fluctuations in pyrochlore XY antiferromagnets

Conclusive evidence of order by disorder is scarce in real materials. Perhaps one of the strongest cases presented has been for the pyrochlore XY antiferromagnet Er sub(2) Ti super(2) O sub(7), with the ground state selection proceeding by order by disorder induced through the effects of quantum flu...

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Veröffentlicht in:Physical review. B 2016-05, Vol.93 (18), Article 184408
Hauptverfasser: Rau, Jeffrey G., Petit, Sylvain, Gingras, Michel J. P.
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Sprache:eng
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Zusammenfassung:Conclusive evidence of order by disorder is scarce in real materials. Perhaps one of the strongest cases presented has been for the pyrochlore XY antiferromagnet Er sub(2) Ti super(2) O sub(7), with the ground state selection proceeding by order by disorder induced through the effects of quantum fluctuations. This identification assumes the smallness of the effect of virtual crystal field fluctuations that could provide an alternative route to picking the ground state. Here we show that this order by virtual crystal field fluctuations is not only significant, but competitive with the effects of quantum fluctuations. Further, we argue that higher-multipolar interactions that are generically present in rare-earth magnets can dramatically enhance this effect. From a simplified bilinear-biquadratic model of these multipolar interactions, we show how the virtual crystal field fluctuations manifest in Er sub(2) Ti sub(2) O sub(7) using a combination of strong-coupling perturbation theory and the random-phase approximation. We find that the experimentally observed [psi] sub(2) state is indeed selected and the experimentally measured excitation gap can be reproduced when the bilinear and biquadratic couplings are comparable while maintaining agreement with the entire experimental spin-wave excitation spectrum. Finally, we comment on possible tests of this scenario and discuss implications for other order-by-disorder candidates in rare-earth magnets.
ISSN:2469-9950
2469-9969
DOI:10.1103/PhysRevB.93.184408