127,987 research outputs found

    D-outcome measurement for a nonlocality test

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    For the purpose of the nonlocality test, we propose a general correlation observable of two parties by utilizing local dd-outcome measurements with SU(dd) transformations and classical communications. Generic symmetries of the SU(dd) transformations and correlation observables are found for the test of nonlocality. It is shown that these symmetries dramatically reduce the number of numerical variables, which is important for numerical analysis of nonlocality. A linear combination of the correlation observables, which is reduced to the Clauser-Horne-Shimony-Holt (CHSH) Bell's inequality for two outcome measurements, is led to the Collins-Gisin-Linden-Massar-Popescu (CGLMP) nonlocality test for dd-outcome measurement. As a system to be tested for its nonlocality, we investigate a continuous-variable (CV) entangled state with dd measurement outcomes. It allows the comparison of nonlocality based on different numbers of measurement outcomes on one physical system. In our example of the CV state, we find that a pure entangled state of any degree violates Bell's inequality for d(2)d(\ge 2) measurement outcomes when the observables are of SU(dd) transformations.Comment: 16 pages, 2 figure

    A New SX Phe Star in the Globular Cluster M15

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    A new SX Phe star (labelled SXP1) found from BVBV CCD photometry is the first to be discovered in the globular cluster M15. It is a blue straggler and is located 102\arcsec.8 north and 285\arcsec.6 west of the center of M15 \citep{har96}. Mean magnitudes of SXP1 are = 18$\fm$671 and = 18\fm445. The amplitude of variability of SXP1 is measured to be ΔV0.15\Delta V \approx 0.15. From multiple-frequency analysis based on the Fourier decomposition method, we detect two very closely separated pulsating frequencies: the primary frequency at f1=24.630f_1=24.630 c/d for both BB- and VV-bands, and the secondary frequency at f2=24.338f_2=24.338 c/d for the BB-band and 24.343 c/d for the VV-band. This star is the second among known SX Phe stars found to pulsate with very closely separated frequencies (f2/f10.95f_2/f_1\ge0.95). These frequencies may be explained by excitation of nonradial modes; however, we have an incomplete understanding of this phenomenon in the case of SX Phe stars with relatively high amplitudes. The metallicity-period and the variability amplitude-period relations for SXP1 in M15 are found to be consistent with those for SX Phe stars in other globular clusters.Comment: 15 pages with 6 figures, accepted by the Astronomical Journal (scheduled May 2001

    Demonstration of nanoimprinted hyperlens array for high-throughput sub-diffraction imaging

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    Partial Teleportation of Entanglement in the Noisy Environment

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    Partial teleportation of entanglement is to teleport one particle of an entangled pair through a quantum channel. This is conceptually equivalent to quantum swapping. We consider the partial teleportation of entanglement in the noisy environment, employing the Werner-state representation of the noisy channel for the simplicity of calculation. To have the insight of the many-body teleportation, we introduce the measure of correlation information and study the transfer of the correlation information and entanglement. We find that the fidelity gets smaller as the initial-state is entangled more for a given entanglement of the quantum channel. The entangled channel transfers at least some of the entanglement to the final state.Comment: 8 pages, 2 figure
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