2,157 research outputs found

    Research in the development effort of an improved multiplier phototube Seventh quarterly report

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    Test data on effective photocathode size, response uniformity, and pulse amplitude distribution of multiplier phototube

    Research in the development of an improved multiplier phototube Final report

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    Cascade aperture design, gas pressure effects, gain calibration, and photon counting efficiency of multiplier phototub

    Research in the development of an improved multiplier phototube Final report

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    Counting efficiency, noise factor measurement, dark noise, gain and counting rate, optical enhancemen

    Research in the development of an improved multiplier phototube

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    Performance and response characteristics of smoothing, image intensifier dissector for low light level astronomy and optical detectio

    Research in the development of an improved multiplier phototube

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    Parameters in analog /dc/ and digital /single electron pulse count/ modes of processing data from photomultiplier tube

    Research in the development effort of an improved multiplier phototube third quarterly report

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    First dynode gain mapping for improving multiplier phototub

    Dual Behavior of Antiferromagnetic Uncompensated Spins in NiFe/IrMn Exchange Biased Bilayers

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    We present a comprehensive study of the exchange bias effect in a model system. Through numerical analysis of the exchange bias and coercive fields as a function of the antiferromagnetic layer thickness we deduce the absolute value of the averaged anisotropy constant of the antiferromagnet. We show that the anisotropy of IrMn exhibits a finite size effect as a function of thickness. The interfacial spin disorder involved in the data analysis is further supported by the observation of the dual behavior of the interfacial uncompensated spins. Utilizing soft x-ray resonant magnetic reflectometry we have observed that the antiferromagnetic uncompensated spins are dominantly frozen with nearly no rotating spins due to the chemical intermixing, which correlates to the inferred mechanism for the exchange bias.Comment: 4 pages, 3 figure

    Research in the development of an improved multiplier phototube Final report

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    Triggered light sources, after pulsing, and materials for multiplier phototube

    N∗N^{\bf *} decays to NωN\omega from new data on γp→ωp\gamma p\to \omega p

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    Data on the reaction γp→ωp\gamma p\to \omega p with ω→π0γ\omega\to\pi^0\gamma, taken with unpolarized or polarized beams in combination with an unpolarized or polarized proton-target, were analyzed within the Bonn-Gatchina (BnGa) partial wave analysis. Differential cross sections, several spin density matrix elements, the beam asymmetry Σ\Sigma, the normalized helicity difference EE, and the correlation GG between linear photon and longitudinal target polarization were included in a large data base on pion and photo-induced reactions. The data on ω\omega photoproduction are used to determine twelve N∗→NωN^*\to N\omega branching ratios; most of these are determined for the first time.Comment: 6 pages, 4 figures, 2 table

    The formation of Uranus and Neptune among Jupiter and Saturn

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    The outer giant planets, Uranus and Neptune, pose a challenge to theories of planet formation. They exist in a region of the Solar System where long dynamical timescales and a low primordial density of material would have conspired to make the formation of such large bodies (∼\sim 15 and 17 times as massive as the Earth, respectively) very difficult. Previously, we proposed a model which addresses this problem: Instead of forming in the trans-Saturnian region, Uranus and Neptune underwent most of their growth among proto-Jupiter and -Saturn, were scattered outward when Jupiter acquired its massive gas envelope, and subsequently evolved toward their present orbits. We present the results of additional numerical simulations, which further demonstrate that the model readily produces analogues to our Solar System for a wide range of initial conditions. We also find that this mechanism may partly account for the high orbital inclinations observed in the Kuiper belt.Comment: Submitted to AJ; 38 pages, 16 figure
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