163,400 research outputs found

    Cupric chloride CuCl2 as an S=1/2 chain multiferroic

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    Magnetoelectric properties were investigated for an S=1/2 chain antiferromagnet CuCl2, which turns out to be the first example of non-chalcogen based spiral-spin induced multiferroics. Upon the onset of helimagnetic order propagating along the b-axis under zero magnetic field (H), we found emergence of ferroelectric polarization along the c-axis. Application of H along the b-axis leads to spin-flop transition coupled with drastic suppression of ferroelectricity, and rotation of H around the b-axis induces the rotation of spin-spiral plane and associated polarization direction. These behaviors are explained well within the framework of the inverse Dzyaloshinskii-Moriya model, suggesting the robustness of this magnetoelectric coupling mechanism even under the strong quantum fluctuation.Comment: 5 pages, 5 figure

    Grease lubricated spiral groove gyro bearings Final report

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    Grease lubricated spiral groove bearings suitable for spin axis of gyros in automatic pilot

    Method to measure off-axis displacements based on the analysis of the intensity distribution of a vortex beam

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    We study the properties of the Fraunhofer diffraction patterns produced by Gaussian beams crossing spiral phase plates. We show, both analytically and numerically, that off-axis displacements of the input beam produce asymmetric diffraction patterns. The intensity profile along the direction of maximum asymmetry shows two different peaks. We find that the intensity ratio between these two peaks decreases exponentially with the off-axis displacement of the incident beam, the decay being steeper for higher strengths of the optical singularity of the spiral phase plate. We analyze how this intensity ratio can be used to measure small misalignments of the input beam with a very high precision.Comment: 8 pages, 4 figures. Accepted for publication in PR

    Dynamics of Gaseous Disks in a Non-axisymmetric Dark Halo

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    The dynamics of a galactic disk in a non-axisymmetric (triaxial) dark halo is studied in detail using high-resolution, numerical, hydrodynamical models. A long-lived, two-armed spiral pattern is generated for a wide range of parameters. The spiral structure is global, and the number of turns can be two or three, depending on the model parameters. The morphology and kinematics of the spiral pattern are studied as functions of the halo and disk parameters. The spiral structure rotates slowly, and its angular velocity varies quasi-periodically. Models with differing relative halo masses, halo semi-axis ratios, distributions of matter in the disk, Mach numbers in the gaseous component, and angular rotational velocities of their halos are considered.Comment: 22 pages, 11 figure

    Subaru/HiCIAO HKsHK_{\rm s} imaging of LkHα\alpha 330 - multi-band detection of the gap and spiral-like structures

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    We present HH- and KsK_{\rm s}-bands observations of the LkHα\alpha 330 disk with a multi-band detection of the large gap and spiral-like structures. The morphology of the outer disk (rr\sim0\farcs3) at PA=0--45^\circ and PA=180--290^\circ are likely density wave-induced spirals and comparison between our observational results and simulations suggests a planet formation. We have also investigated the azimuthal profiles at the ring and the outer-disk regions as well as radial profiles in the directions of the spiral-like structures and semi-major axis. Azimuthal analysis shows a large variety in wavelength and implies that the disk has non-axisymmetric dust distributions. The radial profiles in the major-axis direction (PA=271271^\circ) suggest that the outer region (r\geq0\farcs25) may be influenced by shadows of the inner region of the disk. The spiral-like directions (PA=10^\circ and 230^\circ) show different radial profiles, which suggests that the surfaces of the spiral-like structures are highly flared and/or have different dust properties. Finally, a color-map of the disk shows a lack of an outer eastern region in the HH-band disk, which may hint the presence of an inner object that casts a directional shadow onto the disk.Comment: 12pages, 16 figures, 2 tables, accepted for publication in A
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