2008
DOI: 10.1088/0953-8984/20/23/235222
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Heat capacity and thermal expansion of the itinerant helimagnet MnSi

Abstract: The heat capacity and thermal expansion of a high quality single crystal of MnSi were measured at ambient pressure at zero and high magnetic fields. The calculated magnetic entropy change in the temperature range 0-30 K is less than 0.1R, a low value that emphasizes the itinerant nature of magnetism in MnSi. A linear temperature term dominates the thermal expansion coefficient in the range 30-150 K, which correlates with an enhancement of the linear electronic term in the heat capacity. A surprising similarity… Show more

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Cited by 70 publications
(88 citation statements)
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“…Meanwhile a careful study of the magnetic phase transition in MnSi confirmed a first order nature of the transition at least at ambient pressure 4,5,6 , as was proposed long ago in Ref.…”
supporting
confidence: 61%
“…Meanwhile a careful study of the magnetic phase transition in MnSi confirmed a first order nature of the transition at least at ambient pressure 4,5,6 , as was proposed long ago in Ref.…”
supporting
confidence: 61%
“…10,11 Experimentally, there has been a large number of works dealing with the spin resistivity in different magnetic compounds. 12,13,14,15,16,17,18,19,20,21,22 These experiments show the existence of an anomaly of ρ at the magnetic phase transition. The shape of this anomaly depends on the material.…”
Section: Introductionmentioning
confidence: 70%
“…35 Si 58.8 [4] 0.218 [4] 4.471 [19] 471 [5] 0.145 [4] (a) orders antiferromagnetically; (b) interpolated value using data in Ref [8].…”
Section: Introductionmentioning
confidence: 99%
“…The sense of the magnetization rotation is fixed due to the presence of the chiral DzyaloshinskiiMoriya (DM) interaction [20,21]. However, in their magnetic field−temperature, (H, T ), phase diagrams, as sketched in figure 1(a), numerous puzzling physical anomalies have been observed in a narrow temperature interval in the vicinity of T C [8,10,22,23,24,25,26,27,28,29,30,31,32,33,34,35,36,37,38,39,40,41,42]. The origin of these "precursor anomalies" (hatched area in figure 1(a)) and notably the magnetic structure of the so-called A phase is a long-standing and intriguing problem in chiral magnetism.…”
Section: Introductionmentioning
confidence: 99%