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The pressure effect on the Nèel temperature TN of DyB6 has been investigated by measuring the temperature dependence of electrical resistivity (ρ) at various pressures up to 8 GPa. It was found that TN increases almost linearly with pressure in the range of 0-2 GPa and then tends to saturate above 2 GPa. The pressure derivative of TN below 2 GPa was estimated to be 2.6 K/GPa. The pressure effect on the volume of DyB6 has also been measured at high pressure up to 14 GPa at room temperature using X-ray diffraction and diamond anvil cell. The pressure dependence of volume of LaB6 was also measured for the comparison. It is revealed that DyB6 is more compressible than LaB6. The origin for this observation is suggested to be due to the difference of the ionic size of the rare earth elements, or the strong electron-phonon interaction in DyB6. [ABSTRACT FROM AUTHOR]

The pressure effect on the Nèel temperature TN of DyB6 has been investigated by measuring the temperature dependence of electrical resistivity (ρ) at various pressures up to 8 GPa. It was found that TN increases almost linearly with pressure in the range of 0-2 GPa and then tends to saturate above 2 GPa. The pressure derivative of TN below 2 GPa was estimated to be 2.6 K/GPa. The pressure effect on the volume of DyB6 has also been measured at high pressure up to 14 GPa at room temperature using X-ray diffraction and diamond anvil cell. The pressure dependence of volume of LaB6 was also measured for the comparison. It is revealed that DyB6 is more compressible than LaB6. The origin for this observation is suggested to be due to the difference of the ionic size of the rare earth elements, or the strong electron-phonon interaction in DyB6. [ABSTRACT FROM AUTHOR]

Experimental investigations into the field dependence of magnetization and temperature dependences of magnetic susceptibility in Ni 2+ x MnGa 1- x ( x = 0.00, 0.02, 0.04) and Co₂VGa Heusler alloy ferromagnets were performed following the spin fluctuation theory of itinerant ferromagnetism, called as "Takahashi theory". We investigated the magnetic field dependence of magnetization at the Curie temperature T C , which is the critical temperature of the ferromagnetic⁻paramagnetic transition, and also at T = 5 K, which concerns the ground state of the ferromagnetic state. The field dependence of the magnetization was analyzed by means of the H vs. M ⁵ dependence, and the field dependence of the ground state at 5 K was investigated by means of an Arrott plot ( H/M vs. M ²) according to the Takahashi theory. As for Ni 2+ x MnGa 1- x , the spin fluctuation parameter in k -space (momentum space, T A ) and that in energy space ( T ₀) obtained at T C and 5 K were almost the same. On the contrary, as for Co₂VGa, the H vs. M ⁵ dependence was not shown at T C . We obtained T A and T ₀ by means of an Arrott plot at 5 K. We created a generalized Rhodes⁻Wohlfarth plot of p eff / p S versus T C / T ₀ for the other ferromagnets. The plot indicated that the relationship between p eff / p S and T ₀/ T C followed Takahashi's theory. We also discussed the spontaneous magnetic moment at the ground state, p S , which was obtained by an Arrott plot at 5 K and the high temperature magnetic moment, p C , at the paramagnetic phase. As for the localized ferromagnet, the p C / p S was 1. As for weak ferromagnets, the p C / p S was larger than 1. In contrast, the p C / p S was smaller than 1 by many Heusler alloys. This is a unique property of Heusler ferromagnets. Half-metallic ferromagnets of Co₂VGa and Co₂MnGa were in accordance with the generalized Rhodes⁻Wohlfarth plot with a k m around 1.4. The magnetic properties of the itinerant electron of these two alloys appeared in the majority bands and was confirmed by Takahashi's theory.

Experimental investigations into the field dependence of magnetization and the relationship between magnetization and magnetostriction in Ni 2+x MnGa 1-x (x = 0.00, 0.02, 0.04) alloy ferromagnets were performed following the self-consistent renormalization (SCR) spin fluctuation theory of itinerant ferromagnetism. In this study, we investigated the magnetization of and magnetostriction on Ni 2+x MnGa 1-x ( x = 0.02, 0.04) to check whether these relations held when the ratio of Ni to Ga and, the valence electron concentration per atom, e / a were varied. When the ratio of Ni to Ga was varied, e/a increased with increasing x. The magnetization results for x = 0.02 ( e / a = 7.535) and 0.04 ( e / a = 7.570) suggest that the critical index δ of H ∝ M δ is around 5.0 at the Curie temperature T C , which is the critical temperature of the ferromagnetic⁻paramagnetic transition. This result confirms Takahashi's spin fluctuation theory and the experimental results of Ni₂MnGa. The spontaneous magnetization p S slightly decreased with increasing x . For x = 0.00, the spin fluctuation parameter in k -space (momentum space; T A ) and that in energy space ( T ₀) were obtained. The relationship between p eff / p S and T C / T ₀ can also be explained by Takahashi's theory, where p eff indicates the effective magnetic moments. We created a generalized Rhodes-Wohlfarth plot of p eff / p S versus T C / T ₀ for other ferromagnets. The plot indicates that the relationship between p eff / p S and T ₀/ T C follows Takahashi's theory. We also measured the magnetostriction for Ni 2+x MnGa 1-x (x = 0.02, 0.04). As a result, at T C , the plot of the magnetostriction (Δ L / L ) versus M ⁴ shows proportionality and crosses the origin. These magnetization and magnetostriction results were analyzed in terms of Takahashi's SCR spin fluctuation theory. We investigated the magnetostriction at the premartensite phase, which is the precursor state to the martensitic transition. In Ni₂MnGa system alloys, the maximum value of magnetostriction is almost proportional to the e / a ., Competing Interests: The authors declare no conflict of interest.