1994
DOI: 10.1103/physrevb.49.15730
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X-ray- and neutron-scattering measurements of two length scales in the magnetic critical fluctuations of holmium

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Cited by 61 publications
(53 citation statements)
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“…with small discontinuities. The results are summarized in Tables I and II [108] 0.37(10) [109] 0.39(3) [110] 0.39(2) [111] 0.39(4) [112] 0.39(4) [112] 0.41(4) [113] 1.14(10) 0.57(4) [114] 0.38(1) Dy [115] 0.335(10) [116] 0 We highlight four striking characteristics [118] of these data. Their consequences for the physics of frustrated magnets will be discussed in more details in the following.…”
Section: The Experimental Situationmentioning
confidence: 98%
“…with small discontinuities. The results are summarized in Tables I and II [108] 0.37(10) [109] 0.39(3) [110] 0.39(2) [111] 0.39(4) [112] 0.39(4) [112] 0.41(4) [113] 1.14(10) 0.57(4) [114] 0.38(1) Dy [115] 0.335(10) [116] 0 We highlight four striking characteristics [118] of these data. Their consequences for the physics of frustrated magnets will be discussed in more details in the following.…”
Section: The Experimental Situationmentioning
confidence: 98%
“…In fact, experimental situation concerning the critical properties of these rare-earth helimagnets has remained confused for years now, in the sense that different authors reported significantly different exponent values, or even different order of the transition, for the same exponent of the same material. For example, the reported values of the exponent β are scattered from 0.21 (Tb; X-ray) [13], 0.23 (Tb; neutron) [14], 0.25(Tb; neutron) [9], 0.3(Ho; neutron) [15], 0.335(Dy; Mösbauer) [8], 0.37(Ho; X-ray) [16], 0.38(Dy; neutron) [17], 0.39(Ho; neutron) [18] to 0.39(Dy; neutron) [18].…”
Section: (B) Chiralitymentioning
confidence: 99%
“…Furthermore, it has been shown at least in Ho [10] and SrTiO 3 [11,12] that the NC is sample dependent, and that its critical behavior is different from that of the BC, with larger critical exponents. The NC component was found to depend on surface preparation [12,13], and to arise from a near surface skin region (typically 10 to 100 µm-thick).…”
mentioning
confidence: 99%
“…Longrange strains are believed to be due to dislocation dipoles, at least in Ho (Ref. [10]) and Tb (Ref. [25]).…”
mentioning
confidence: 99%