5,580 research outputs found

    Electronic Structures of Antiperovskite Superconductor MgCNi3_3 and Related Compounds

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    Electronic structure of a newly discovered antiperovskite superconductor MgCNi3_3 is investigated by using the LMTO band method. The main contribution to the density of states (DOS) at the Fermi energy EFE_{\rm F} comes from Ni 3dd states which are hybridized with C 2pp states. The DOS at EFE_{\rm F} is varied substantially by the hole or electron doping due to the very high and narrow DOS peak located just below EFE_{\rm F}. We have also explored electronic structures of C-site and Mg-site doped MgCNi3_3 systems, and described the superconductivity in terms of the conventional phonon mechanism.Comment: 3 pages, presented at ORBITAL2001 September 11-14, 2001 (Sendai, JAPAN

    Electronic structures of antiperovskite superconductors: MgXNi3_3 (X=B,C,N)

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    We have investigated electronic structures of a newly discovered antiperovskite superconductor MgCNi3_3 and related compounds MgBNi3_3 and MgNNi3_3. In MgCNi3_3, a peak of very narrow and high density of states is located just below EF\rm E_F, which corresponds to the π\pi^* antibonding state of Ni-3d and C-2p2p but with the predominant Ni-3d character. The prominent nesting feature is observed in the Γ\Gamma-centered electron Fermi surface of an octahedron-cage-like shape that originates from the 19th band. The estimated superconducting parameters based on the simple rigid-ion approximation are in reasonable agreement with experiment, suggesting that the superconductivity in MgCNi3_3 is described well by the conventional phonon mechanism.Comment: 5 pages, 5 figure

    Electronic structure of metallic antiperovskite compound GaCMn3_3

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    We have investigated electronic structures of antiperovskite GaCMn3_3 and related Mn compounds SnCMn3_3, ZnCMn3_3, and ZnNMn3_3. In the paramagnetic state of GaCMn3_3, the Fermi surface nesting feature along the ΓR\Gamma{\rm R} direction is observed, which induces the antiferromagnetic (AFM) spin ordering with the nesting vector {\bf Q} ΓR\sim \Gamma{\rm R}. Calculated susceptibilities confirm the nesting scenario for GaCMn3_3 and also explain various magnetic structures of other antiperovskite compounds. Through the band folding effect, the AFM phase of GaCMn3_3 is stabilized. Nearly equal densities of states at the Fermi level in the ferromagnetic and AFM phases of GaCMn3_3 indicate that two phases are competing in the ground state.Comment: 4 pages, 5 figure

    Spin-Orbit Qubits of Rare-Earth-Metal Ions in Axially Symmetric Crystal Fields

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    Contrary to the well known spin qubits, rare-earth qubits are characterized by a strong influence of crystal field due to large spin-orbit coupling. At low temperature and in the presence of resonance microwaves, it is the magnetic moment of the crystal-field ground-state which nutates (for several μ\mus) and the Rabi frequency ΩR\Omega_R is anisotropic. Here, we present a study of the variations of ΩR(H0)\Omega_R(\vec{H}_{0}) with the magnitude and direction of the static magnetic field H0\vec{H_{0}} for the odd 167^{167}Er isotope in a single crystal CaWO4_4:Er3+^{3+}. The hyperfine interactions split the ΩR(H0)\Omega_R(\vec{H}_{0}) curve into eight different curves which are fitted numerically and described analytically. These "spin-orbit qubits" should allow detailed studies of decoherence mechanisms which become relevant at high temperature and open new ways for qubit addressing using properly oriented magnetic fields

    Massive gravity wrapped in the cosmic web

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    We study how the filamentary pattern of the cosmic web changes if the true gravity deviates from general relativity (GR) on a large scale. The f(R) gravity, whose strength is controlled to satisfy the current observational constraints on the cluster scale, is adopted as our fiducial model and a large, high-resolution N-body simulation is utilized for this study. By applying the minimal spanning tree algorithm to the halo catalogs from the simulation at various epochs, we identify the main stems of the rich superclusters located in the most prominent filamentary section of the cosmic web and determine their spatial extents per member cluster to be the degree of their straightness. It is found that the f(R) gravity has the effect of significantly bending the superclusters and that the effect becomes stronger as the universe evolves. Even in the case where the deviation from GR is too small to be detectable by any other observables, the degree of the supercluster straightness exhibits a conspicuous difference between the f(R) and the GR models. Our results also imply that the supercluster straightness could be a useful discriminator of f(R) gravity from the coupled dark energy since it is shown to evolve differently between the two models. As a final conclusion, the degree of the straightness of the rich superclusters should provide a powerful cosmological test of large scale gravity

    Analytic study of the urn model for separation of sand

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    We present an analytic study of the urn model for separation of sand recently introduced by Lipowski and Droz (Phys. Rev. E 65, 031307 (2002)). We solve analytically the master equation and the first-passage problem. The analytic results confirm the numerical results obtained by Lipowski and Droz. We find that the stationary probability distribution and the shortest one among the characteristic times are governed by the same free energy. We also analytically derive the form of the critical probability distribution on the critical line, which supports their results obtained by numerically calculating Binder cumulants (cond-mat/0201472).Comment: 6 pages including 3 figures, RevTe

    Analytic study of the three-urn model for separation of sand

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    We present an analytic study of the three-urn model for separation of sand. We solve analytically the master equation and the first-passage problem. We find that the stationary probability distribution obeys the detailed balance and is governed by the {\it free energy}. We find that the characteristic lifetime of a cluster diverges algebraically with exponent 1/3 at the limit of stability.Comment: 5pages, 4 figures include
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