18,955 research outputs found

    Low loss dichroic plate

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    A low loss dichroic plate is disclosed for passing radiation within a particular frequency band and reflecting radiation outside of that frequency band. The dichroic plate is comprised of a configuration of dipole elements defined by slots formed in a conductive plate. The slots are dimensioned so as to pass radiation of a selected frequency and are shaped so as to minimize the relationship between that frequency and the tilt angle of the plate relative to the direction of radiation. The slots are arranged so as to minimize signal power loss due to cross polarization effects

    Low-loss, circularly-polarized dichroic plate

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    Dichroic plate has orthogonally-disposed, loaded dipole apertures with their orientations arranged so as to cancel cross-coupling effects which would otherwise result in power loss to circularly polarized signal

    Tree-level electron-photon interactions in graphene

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    Graphene's low-energy electronic excitations obey a 2+1 dimensional Dirac Hamiltonian. After extending this Hamiltonian to include interactions with a quantized electromagnetic field, we calculate the amplitude associated with the simplest, tree-level Feynman diagram: the vertex connecting a photon with two electrons. This amplitude leads to analytic expressions for the 3D angular dependence of photon emission, the photon-mediated electron-hole recombination rate, and corrections to graphene's opacity πα\pi \alpha and dynamic conductivity πe2/2h\pi e^2/2 h for situations away from thermal equilibrium, as would occur in a graphene laser. We find that Ohmic dissipation in perfect graphene can be attributed to spontaneous emission.Comment: 5 pages, 3 figure

    Effect of ferromagnetic contacts on spin accumulation in an all-metallic lateral spin-valve system: Semiclassical spin drift-diffusion equations

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    We study the effect of the ferromagnetic (FM) contacts on the spin accumulation in the lateral spin valve system for the collinear magnetization configurations. When an additional FM electrode is introduced in the all-metallic lateral spin-valve system, we find that the transresistance can be fractionally suppressed or very weakly influenced depending on the position of the additional FM electrode, and relative magnitudes of contact resistance and the bulk resistance defined over the spin diffusion length. Nonlocal spin signals such as nonlocal voltage drop and leakage spin currents are independent of the magnetization orientation of the additional FM electrode. Even when the additional contact is nonmagnetic, nonlocal spin signals can be changed by the spin current leaking into the nonmagnetic electrode.Comment: 13 pages, 1 figure, revised versio

    A finite element-boundary integral method for conformal antenna arrays on a circular cylinder

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    Conformal antenna arrays offer many cost and weight advantages over conventional antenna systems. In the past, antenna designers have had to resort to expensive measurements in order to develop a conformal array design. This is due to the lack of rigorous mathematical models for conformal antenna arrays, and as a result the design of conformal arrays is primarily based on planar antenna design concepts. Recently, we have found the finite element-boundary integral method to be very successful in modeling large planar arrays of arbitrary composition in a metallic plane. Herewith we shall extend this formulation for conformal arrays on large metallic cylinders. In this we develop the mathematical formulation. In particular we discuss the finite element equations, the shape elements, and the boundary integral evaluation, and it is shown how this formulation can be applied with minimal computation and memory requirements. The implementation shall be discussed in a later report

    Nearly Deterministic Bell Measurement for Multiphoton Qubits and Its Application to Quantum Information Processing

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    We propose a Bell measurement scheme by employing a logical qubit in Greenberger-Horne-Zeilinger (GHZ) entanglement with an arbitrary number of photons. Remarkably, the success probability of the Bell measurement as well as teleportation of the GHZ entanglement can be made arbitrarily high using only linear optics elements and photon on-off measurements as the number of photons increases. Our scheme outperforms previous proposals using single photon qubits when comparing the success probabilities in terms of the average photon usages. It has another important advantage for experimental feasibility that it does not require photon number resolving measurements. Our proposal provides an alternative candidate for all-optical quantum information processing.Comment: 7 pages (including supplementary material), 2 figures, to be published in Phys. Rev. Let

    Two Conditions for Galaxy Quenching: Compact Centres and Massive Haloes

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    We investigate the roles of two classes of quenching mechanisms for central and satellite galaxies in the SDSS (z<0.075z<0.075): those involving the halo and those involving the formation of a compact centre. For central galaxies with inner compactness Σ1kpc1099.4Mkpc2\Sigma_{\rm 1kpc} \sim 10^{9-9.4}M_{\odot} {\rm kpc}^{-2}, the quenched fraction fqf_{q} is strongly correlated with Σ1kpc\Sigma_{\rm 1kpc} with only weak halo mass MhM_{\rm h} dependence. However, at higher and lower Σ1kpc\Sigma_{\rm 1kpc}, sSFR is a strong function of MhM_{\rm h} and mostly independent of Σ1kpc\Sigma_{\rm 1kpc}. In other words, Σ1kpc1099.4Mkpc2\Sigma_{\rm 1kpc} \sim 10^{9-9.4} M_{\odot} {\rm kpc}^{-2} divides galaxies into those with high sSFR below and low sSFR above this range. In both the upper and lower regimes, increasing MhM_{\rm h} shifts the entire sSFR distribtuion to lower sSFR without a qualitative change in shape. This is true even at fixed MM_{*}, but varying MM_{*} at fixed MhM_{\rm h} adds no quenching information. Most of the quenched centrals with Mh>1011.8MM_{\rm h} > 10^{11.8}M_{\odot} are dense (Σ1kpc>109 Mkpc2\Sigma_{\rm 1kpc} > 10^{9}~ M_{\odot} {\rm kpc}^{-2}), suggesting compaction-related quenching maintained by halo-related quenching. However, 21% are diffuse, indicating only halo quenching. For satellite galaxies in the outskirts of halos, quenching is a strong function of compactness and a weak function of host MhM_{\rm h}. In the inner halo, MhM_{\rm h} dominates quenching, with 90%\sim 90\% of the satellites being quenched once Mh>1013MM_{\rm h} > 10^{13}M_{\odot}. This regional effect is greatest for the least massive satellites. As demonstrated via semi-analytic modelling with simple prescriptions for quenching, the observed correlations can be explained if quenching due to central compactness is rapid while quenching due to halo mass is slow.Comment: 16 pages, 11 figures, MNRAS accepte
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