692 research outputs found

    Elasticity-mediated self-organization and colloidal interactions of solid spheres with tangential anchoring in a nematic liquid crystal

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    Using laser tweezers and fluorescence confocal polarizing microscopy, we study colloidal interactions of solid microspheres in the nematic bulk caused by elastic distortions around the particles with strong tangential surface anchoring. The particles aggregate into chains directed at about 30 degrees to the far field director and, at higher concentrations, form complex kinetically trapped structures. We characterize the distance and angular dependencies of the colloidal interaction forces.Comment: 6 pages, 5 figure

    Von Neumann Entropy-Preserving Quantum Operations

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    For a given quantum state ρ\rho and two quantum operations Φ\Phi and Ψ\Psi, the information encoded in the quantum state ρ\rho is quantified by its von Neumann entropy §(ρ)\S(\rho). By the famous Choi-Jamio{\l}kowski isomorphism, the quantum operation Φ\Phi can be transformed into a bipartite state, the von Neumann entropy §map(Φ)\S^{\mathrm{map}}(\Phi) of the bipartite state describes the decoherence induced by Φ\Phi. In this Letter, we characterize not only the pairs (Φ,ρ)(\Phi, \rho) which satisfy §(Φ(ρ))=§(ρ)\S(\Phi(\rho))=\S(\rho), but also the pairs (Φ,Ψ)(\Phi, \Psi) which satisfy §map(ΦΨ)=§map(Ψ)\S^{\mathrm{map}}(\Phi\circ\Psi) = \S^{\mathrm{map}}(\Psi).Comment: 7 pages, LaTeX, to appear Phys. Lett.

    Theory of wind accretion

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    A review of wind accretion in high-mass X-ray binaries is presented. We focus attention to different regimes of quasi-spherical accretion onto the neutron star: the supersonic (Bondi) accretion, which takes place when the captured matter cools down rapidly and falls supersonically toward NS magnetospghere, and subsonic (settling) accretion which occurs when plasma remains hot until it meets the magnetospheric boundary. Two regimes of accretion are separated by an X-ray luminosity of about 4×10364\times10^{36} erg/s. In the subsonic case, which sets in at low luminosities, a hot quasi-spherical shell must be formed around the magnetosphere, and the actual accretion rate onto NS is determined by ability of the plasma to enter the magnetosphere due to Rayleigh-Taylor instability. We calculate the rate of plasma entry the magnetopshere and the angular momentum transfer in the shell due to turbulent viscosity appearing in the convective differentially rotating shell. We also discuss and calculate the structure of the magnetospheric boundary layer where the angular momentum between the rotating magnetosphere and the base of the differentially rotating quasi-spherical shell takes place. We show how observations of equilibrium X-ray pulsars Vela X-1 and GX 301-2 can be used to estimate dimensionless parameters of the subsonic settling accretion theory, and obtain the width of the magnetospheric boundary layer for these pulsars.Comment: LaTeX, 10 pages, 5 figures; submitted to Proc. of Int. Conf. "Physics at the Magnetspheric Boundary", Geneva, Switzerland, 25-28 June, 201
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