59,642 research outputs found

    Spin-dependent transport in a quasiballistic quantum wire

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    We describe the transport properties of a 5 μ\mum long one-dimensional (1D) quantum wire. Reduction of conductance plateaux due to the introduction of weakly disorder scattering are observed. In an in-plane magnetic field, we observe spin-splitting of the reduced conductance steps. Our experimental results provide evidence that deviation from conductance quantisation is very small for electrons with spin parallel and is about 1/3 for electrons with spin anti-parallel. Moreover, in a high in-plane magnetic field, a spin-polarised 1D channel shows a plateau-like structure close to 0.3×e2/h0.3 \times e^2/h which strengthens with {\em increasing} temperatures. It is suggested that these results arise from the combination of disorder and the electron-electron interactions in the 1D electron gas.Comment: 4 pages, 5 figures, latex to be published in Phys. Rev. B (15/3/2000

    Quasi-local energy for cosmological models

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    First we briefly review our covariant Hamiltonian approach to quasi-local energy, noting that the Hamiltonian-boundary-term quasi-local energy expressions depend on the chosen boundary conditions and reference configuration. Then we present the quasi-local energy values resulting from the formalism applied to homogeneous Bianchi cosmologies. Finally we consider the quasi-local energies of the FRW cosmologies. Our results do not agree with certain widely accepted quasi-local criteria.Comment: Contributed to International Symposium on Cosmology and Particle Astrophysics (CosPA 2006), Taipei, Taiwan, 15-17 Nov 200

    A New Model for the Hard Time Lags in Black Hole X-Ray Binaries

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    The time-dependent Comptonized output of a cool soft X-ray source drifting inward through an inhomogeneous hot inner disk or corona is numerically simulated. We propose that this scenario can explain from first principles the observed trends in the hard time lags and power spectra of the rapid aperiodic variability of the X-ray emission of Galactic black-hole candidates.Comment: 10 pages, including 2 figures; uses epsf.sty, rotate.sty; accepted for ApJ Letter

    Description of ρ(1700)\rho (1700) as a ρKKˉ\rho K \bar{K} system with the fixed center approximation

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    We study the ρKKˉ\rho K\bar{K} system with an aim to describe the ρ(1700)\rho (1700) resonance. The chiral unitary approach has achieved success in a description of systems of the light hadron sector. With this method, the KKˉK \bar{K} system in the isospin sector I=0I=0, is found to be a dominant component of the f0(980)f_0 (980) resonance. Therefore, by regarding the KKˉK\bar{K} system as a cluster, the f0(980)f_0 (980) resonance, we evaluate the ρKKˉ\rho K\bar{K} system applying the fixed center approximation to the Faddeev equations. We construct the ρK\rho K unitarized amplitude using the chiral unitary approach. As a result, we find a peak in the three-body amplitude around 1739 MeV and a width of about 227 MeV. The effect of the width of ρ\rho and f0(980)f_0 (980) is also discussed. We associate this peak to the ρ(1700)\rho (1700) which has a mass of 1720±201720 \pm 20 MeV and a width of 250±100250 \pm 100 MeV

    Spin Hall effects for cold atoms in a light induced gauge potential

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    We propose an experimental scheme to observe spin Hall effects with cold atoms in a light induced gauge potential. Under an appropriate configuration, the cold atoms moving in a spatially varying laser field experience an effective spin-dependent gauge potential. Through numerical simulation, we demonstrate that such a gauge field leads to observable spin Hall currents under realistic conditions. We also discuss the quantum spin Hall state in an optical lattice.Comment: 4 pages; The published versio
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