638 research outputs found

    Magnetic phase diagram of three-dimensional diluted Ising antiferromagnet Ni0.8_{0.8}Mg0.2_{0.2}(OH)2_{2}

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    HH-TT diagram of 3D diluted Ising antiferromagnet Nic_{c}Mg1c_{1-c}(OH)2_{2} with cc = 0.8 has been determined from measurements of SQUID DC magnetization and AC magnetic susceptibility. At HH = 0, this compound undergoes two magnetic phase transitions: an antiferromagnetic (AF) transition at the N\'{e}el temperature TNT_{N} (= 20.7 K) and a reentrant spin glass (RSG) transition at TRSGT_{RSG} (\approx 6 K). The HH-TT diagram consists of the RSG, spin glass (SG), and AF phases. These phases meet a multicritical point PmP_{m} (HmH_{m} = 42 kOe, TmT_{m} = 5.6 K). The irreversibility of susceptibility defined by δ\delta (= χFCχZFC\chi_{FC} - \chi_{ZFC}) shows a negative local minimum for 10 H\leq H \leq 35 kOe, suggesting the existence of possible glassy phase in the AF phase. A broad peak in δ\delta and χ\chi^{\prime \prime} at HH \geq 20 kOe for TN(c=0.8,H)TTN(c=1,H=0)T_{N}(c=0.8,H) \leq T \leq T_{N}(c=1,H=0) (= 26.4 K) suggests the existence of the Griffiths phase.Comment: 11 pages, 14 figures; J. Phys. Soc. Jpn. 73 (2004) No. 1 issue, in pres

    Gravitational Waves from Supermassive Black Hole Coalescence in a Hierarchical Galaxy Formation Model

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    We investigate the expected gravitational wave emission from coalescing supermassive black hole (SMBH) binaries resulting from mergers of their host galaxies. When galaxies merge, the SMBHs in the host galaxies sink to the center of the new merged galaxy and form a binary system. We employ a semi-analytic model of galaxy and quasar formation based on the hierarchical clustering scenario to estimate the amplitude of the expected stochastic gravitational wave background owing to inspiraling SMBH binaries and bursts owing to the SMBH binary coalescence events. We find that the characteristic strain amplitude of the background radiation is hc(f)1016(f/1μHz)2/3h_c(f) \sim 10^{-16} (f/1 \mu {\rm Hz})^{-2/3} for f1μHzf \lesssim 1 \mu {\rm Hz} just below the detection limit from measurements of the pulsar timing provided that SMBHs coalesce simultaneously when host galaxies merge. The main contribution to the total strain amplitude of the background radiation comes from SMBH coalescence events at 0<z<10<z<1. We also find that a future space-based gravitational wave interferometer such as the planned \textit{Laser Interferometer Space Antenna} ({\sl LISA}) might detect intense gravitational wave bursts associated with coalescence of SMBH binaries with total mass Mtot<107MM_{\rm tot} < 10^7 M_{\odot} at z2z \gtrsim 2 at a rate 1.0yr1 \sim 1.0 {\rm yr}^{-1}. Our model predicts that burst signals with a larger amplitude hburst1015h_{\rm burst} \sim 10^{-15} correspond to coalescence events of massive SMBH binary with total mass Mtot108MM_{\rm tot} \sim 10^8 M_{\odot} at low redshift z1 z \lesssim 1 at a rate 0.1yr1 \sim 0.1 {\rm yr}^{-1} whereas those with a smaller amplitude hburst1017h_{\rm burst} \sim 10^{-17} correspond to coalescence events of less massive SMBH binary with total mass Mtot106MM_{\rm tot} \sim 10^6 M_{\odot} at high redshift z3 z \gtrsim 3.Comment: Accepted for publication in ApJ. 11 pages, 7 figure

    Spin-stripe density varies linearly with hole content in single-layer Bi2201 cuprate

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    We have performed inelastic neutron scattering measurements on the single-layer cuprate Bi2+xSr2-xCuO6+y (Bi2201) with x=0.2, 0.3, 0.4 and 0.5, a doping range that spans the spin-glass (SG) to superconducting (SC) phase boundary. The doping evolution of low energy spin fluctuations was found to be characterized by a change of incommensurate modulation wave vector from the tetragonal [110] to [100]/[010] directions, while maintaining a linear relation between the incommensurability and the hole concentration, delta p. In the SC regime, the spectral weight is strongly suppressed below 4 meV. Similarities and differences in the spin correlations between Bi2201 and the prototypical single-layer system La2-xSrxCuO4 are discussed.Comment: 5 page,4 figure

    Soliton Trap in Strained Graphene Nanoribbons

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    The wavefunction of a massless fermion consists of two chiralities, left-handed and right-handed, which are eigenstates of the chiral operator. The theory of weak interactions of elementally particle physics is not symmetric about the two chiralities, and such a symmetry breaking theory is referred to as a chiral gauge theory. The chiral gauge theory can be applied to the massless Dirac particles of graphene. In this paper we show within the framework of the chiral gauge theory for graphene that a topological soliton exists near the boundary of a graphene nanoribbon in the presence of a strain. This soliton is a zero-energy state connecting two chiralities and is an elementally excitation transporting a pseudospin. The soliton should be observable by means of a scanning tunneling microscopy experiment.Comment: 7 pages, 4 figure

    Extending the linearity range of eddy-current displacement sensor with magnetoplated wire

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    This material is presented to ensure timely dissemination of scholarly and technical work. Copyright and all rights therein are retained by authors or by other copyright holders. All persons copying this information are expected to adhere to the terms and constraints invoked by each author's copyright. In most cases, these works may not be reposted without the explicit permission of the copyright holder.ArticleIEEE TRANSACTIONS ON MAGNETICS. 43(2): 543-548 (2007)journal articl

    Hidden itinerant-spin phase in heavily-overdoped La2-xSrxCuO4 revealed by dilute Fe doping: A combined neutron scattering and angle-resolved photoemission study

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    We demonstrated experimentally a direct way to probe a hidden propensity to the formation of spin density wave (SDW) in a non-magnetic metal with strong Fermi surface nesting. Substituting Fe for a tiny amount of Cu (1%) induced an incommensurate magnetic order below 20 K in heavily-overdoped La2-xSrxCuO4 (LSCO). Elastic neutron scattering suggested that this order cannot be ascribed to the localized spins on Cu or doped Fe. Angle-resolved photoemission spectroscopy (ARPES), combined with numerical calculations, revealed a strong Fermi surface nesting inherent in the pristine LSCO that likely drives this order. The heavily-overdoped Fe-doped LSCO thus represents the first plausible example of the long-sought "itinerant-spin extreme" of cuprates, where the spins of itinerant doped holes define the magnetic ordering ground state. This finding complements the current picture of cuprate spin physics that highlights the predominant role of localized spins at lower dopings. The demonstrated set of methods could potentially apply to studying hidden density-wave instabilities of other "nested" materials on the verge of density wave ordering.Comment: Abstract and discussion revised; to appear in Phys. Rev. Let

    Reduction of eddy current loss in magnetoplated wire

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    ArticleCOMPEL-THE INTERNATIONAL JOURNAL FOR COMPUTATION AND MATHEMATICS IN ELECTRICAL AND ELECTRONIC ENGINEERING. 28(1):57-66 (2009)journal articl

    Reversible Fluorination of Graphene: towards a Two-Dimensional Wide Bandgap Semiconductor

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    We report the synthesis and evidence of graphene fluoride, a two-dimensional wide bandgap semiconductor derived from graphene. Graphene fluoride exhibits hexagonal crystalline order and strongly insulating behavior with resistance exceeding 10 GΩ\Omega at room temperature. Electron transport in graphene fluoride is well described by variable-range hopping in two dimensions due to the presence of localized states in the band gap. Graphene obtained through the reduction of graphene fluoride is highly conductive, exhibiting a resistivity of less than 100 kΩ\Omega at room temperature. Our approach provides a new path to reversibly engineer the band structure and conductivity of graphene for electronic and optical applications.Comment: 7 pages, 5 figures, revtex, to appear in PR

    Reduction of proximity effect in coil using magnetoplated wire

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    This material is presented to ensure timely dissemination of scholarly and technical work. Copyright and all rights therein are retained by authors or by other copyright holders. All persons copying this information are expected to adhere to the terms and constraints invoked by each author's copyright. In most cases, these works may not be reposted without the explicit permission of the copyright holder.ArticleIEEE TRANSACTIONS ON MAGNETICS. 43(6): 2654-2656 (2007)journal articl
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