2011
DOI: 10.1103/physrevb.83.174518
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Low-temperature heat transport of Nd2CuO4: Roles of Nd magnons and spin-structure transitions

Abstract: We report the magnetic-field dependence of thermal conductivity (κ) of an insulating cuprate Nd2CuO4 at very low temperatures down to 0.3 K. It is found that apart from the paramagnetic moments scattering on phonons, the Nd 3+ magnons can act as either heat carriers or phonon scatterers, which strongly depends on the long-range antiferromagnetic transition and the fieldinduced transitions of spin structure. In particular, the Nd 3+ magnons can effectively transport heat in the spin-flopped state of the Nd 3+ s… Show more

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Cited by 24 publications
(69 citation statements)
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“…2 shows the ratios l/W for the two samples, where W is the averaged sample width. 36,41 It is clear that both ratios increase quickly at very low temperatures and are expected to approach 1 below 0.3 K. This estimation tells us that it is not likely that the magnetic excitations in DTO (for examples, magnetic monopoles) can make a sizable contribution to transporting heat, since the experimental κ is even smaller than the phonon term in a boundary scattering limit. It should be pointed out that the magnetic-monopole excitations were believed to be negligible at very low temperatures, because the energy barrier for flipping a spin or creating a pair of magnetic monopoles is about 4.4 K. 42 …”
Section: Resultsmentioning
confidence: 87%
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“…2 shows the ratios l/W for the two samples, where W is the averaged sample width. 36,41 It is clear that both ratios increase quickly at very low temperatures and are expected to approach 1 below 0.3 K. This estimation tells us that it is not likely that the magnetic excitations in DTO (for examples, magnetic monopoles) can make a sizable contribution to transporting heat, since the experimental κ is even smaller than the phonon term in a boundary scattering limit. It should be pointed out that the magnetic-monopole excitations were believed to be negligible at very low temperatures, because the energy barrier for flipping a spin or creating a pair of magnetic monopoles is about 4.4 K. 42 …”
Section: Resultsmentioning
confidence: 87%
“…Using the β value obtained from specific-heat measurements (not shown here), the phonon velocity can be calculated and then the mean free path is obtained from the κ. 36,41 The inset to Fig. 2 shows the ratios l/W for the two samples, where W is the averaged sample width.…”
Section: Resultsmentioning
confidence: 99%
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