2,233 research outputs found

    Incommensurate-Commensurate Magnetic Phase Transition in SmRu2_{2}Al10_{10}

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    Magnetic properties of single crystalline SmRu2_{2}Al10_{10} have been investigated by electrical resistivity, magnetic susceptibility, and specific heat. We have confirmed the successive magnetic phase transitions at TN=12.3T_{\text{N}}=12.3 K and TM=5.6T_{\text{M}}=5.6 K. Resonant x-ray diffraction has also been performed to study the magnetic structures. Below TNT_{\text{N}}, the Sm3+^{3+} moments order in an incommensurate structure with q1=(0,0.759,0)q_1=(0, 0.759, 0). The magnetic moments are oriented along the orthorhombic bb axis, which coincides with the magnetization easy axis in the paramagnetic phase. A very weak third harmonic peak is also observed at q3=(0,0.278,0)q_3=(0, 0.278, 0). The transition at TMT_{\text{M}} is a lock-in transition to the commensurate structure described by q1=(0,0.75,0)q_1=(0, 0.75, 0). A well developed third harmonic peak is observed at q3=(0,0.25,0)q_3=(0, 0.25, 0). From the discussion of the magnetic structure, we propose that the long-range RKKY interaction plays an important role, in addition to the strong nearest neighbor antiferromagnetic interaction.Comment: 11 pages, 12 figures, accepted in PR

    Stable Existence of Phase IV inside Phase II under Pressure in Ce0.8_{0.8}La0.2_{0.2}B6_{6}

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    We investigate the pressure effect of the electrical resistivity and magnetization of Ce0.8_{0.8}La0.2_{0.2}B6_{6}. The situation in which phase IV stably exists inside phase II at H=0 T could be realized by applying a pressure above P1.1P\sim 1.1 GPa. This originates from the fact that the stability of phase II under pressure is larger than those of phases IV and III. The results seem to be difficult to reproduce by taking the four interactions of Γ5u\Gamma_{\mathrm{5u}}-type AFO, OxyO_{xy}-type AFQ, TxyzT_{xyz}-type AFO, and AF exchange into account within a mean-field calculation framework.Comment: 4 pages, 5 figures, to appear in J. Phys. Soc. Jpn. 79 (2010) No.

    Kondo effect in CeXc_{c} (Xc_{c}=S, Se, Te) studied by electrical resistivity under high pressure

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    We have measured the electrical resistivity of cerium monochalcogenices, CeS, CeSe, and CeTe, under high pressures up to 8 GPa. Pressure dependences of the antiferromagnetic ordering temperature TNT_{N}, crystal field splitting, and the lnT\ln T anomaly of the Kondo effect have been studied to cover the whole region from the magnetic ordering regime at low pressure to the Fermi liquid regime at high pressure. TNT_{N} initially increases with increasing pressure, and starts to decrease at high pressure as expected from the Doniach's diagram. Simultaneously, the lnT\ln T behavior in the resistivity is enhanced, indicating the enhancement of the Kondo effect by pressure. It is also characteristic in CeXc_{c} that the crystal field splitting rapidly decreases at a common rate of 12.2-12.2 K/GPa. This leads to the increase in the degeneracy of the ff state and further enhancement of the Kondo effect. It is shown that the pressure dependent degeneracy of the ff state is a key factor to understand the pressure dependence of TNT_{N}, Kondo effect, magnetoresistance, and the peak structure in the temperature dependence of resistivity.Comment: 9 pages, 5 figures, accepted for publication in J. Phys. Soc. Jp

    Polar surface engineering in ultra-thin MgO(111)/Ag(111) -- possibility of metal-insulator transition and magnetism

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    A recent report [Kiguchi {\it et al.}, Phys. Rev. B {\bf 68}, 115402 (2003)] that the (111) surface of 5 MgO layers grown epitaxially on Ag(111) becomes metallic to reduce the electric dipole moment raises a question of what will happen when we have fewer MgO layers. Here we have revealed, first experimentally with electron energy-loss spectroscopy, that MgO(111) remains metallic even when one-layer thick, and theoretically with the density functional theory that the metallization should depend on the nature of the substrate. We further show, with a spin-density functional calculation, that a ferromagnetic instability may be expected for thicker films.Comment: 5 pages, 7 figure
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