111,442 research outputs found

    Magnetically centered liquid column float Patent

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    Magnetically centered liquid column floa

    Health Trainers End of Year Review 1st April 2013 – 31st March 2014

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    A critical assessment of health trainer activity, with particular reference to the most deprived social groups, and a focus on mental health and wellbeing

    Monte Carlo methods and applications for the nuclear shell model

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    The shell-model Monte Carlo (SMMC) technique transforms the traditional nuclear shell-model problem into a path-integral over auxiliary fields. We describe below the method and its applications to four physics issues: calculations of sdpf- shell nuclei, a discussion of electron-capture rates in pf-shell nuclei, exploration of pairing correlations in unstable nuclei, and level densities in rare earth systems.Comment: Proceedings of the Nuclear Structure '98 conference, Gatlinburg, TN, 10-15 August 199

    A study of the effect of measurement errors upon a range controller for an entry vehicle

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    Modified control logic with random-number procedure to determine error effects on range controller of reentry vehicl

    Phase noise in distributed oscillators

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    The phase noise of a distributed oscillator is evaluated very simply by identifying an effective capacitance equal to the total capacitance distributed along the transmission lines. The contributions of the various passive and active noise sources to the total phase noise are calculated revealing several guidelines for improved distributed oscillator designs

    In-State versus Out-of-State Students: The Divergence of Interest between Public Universities and State Governments

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    This paper examines the divergence of interest between universities and state governments concerning standards for admitting in-state versus out-of-state students. We find that public universities set lower minimum admissions standards for in-state than out-of-state applicants, presumably in response to state pressure; while private universities treat both groups equally. However, we also find that favoring in-state applicants goes against states’ long-term financial interest. This is because marginal out-of-state students pay higher tuition than marginal in-state students, pay more in future state taxes, and are equally influenced in whether they locate in the state after graduation by attending public university there

    Low NOx heavy fuel combustor concept program

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    Three simulated coal gas fuels based on hydrogen and carbon monoxide were tested during an experimental evaluation with a rich lean can combustor: these were a simulated Winkler gas, Lurgi gas and Blue Water gas. All three were simulated by mixing together the necessary pure component species, to levels typical of fuel gases produced from coal. The Lurgi gas was also evaluated with ammonia addition. Fuel burning in a rich lean mode was emphasized. Only the Blue Water gas, however, could be operated in such fashion. This showed that the expected NOx signature form could be obtained, although the absolute values of NOx were above the 75 ppm goals for most operating conditions. Lean combustion produced very low NOx well below 75 ppm with the Winkler and Lurgi gases. In addition, these low levels were not significantly impacted by changes in operating conditions

    Baryonic Signatures in Large-Scale Structure

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    We investigate the consequences of a non-negligible baryon fraction for models of structure formation in Cold Dark Matter dominated cosmologies, emphasizing in particular the existence of oscillations in the present-day matter power spectrum. These oscillations are the remnants of acoustic oscillations in the photon-baryon fluid before last scattering. For acceptable values of the cosmological and baryon densities, the oscillations modulate the power by up to 10%, with a `period' in spatial wavenumber which is close to Delta k approximately 0.05/ Mpc. We study the effects of nonlinear evolution on these features, and show that they are erased for k > 0.2 h/ Mpc. At larger scales, the features evolve as expected from second-order perturbation theory: the visibility of the oscillations is affected only weakly by nonlinear evolution. No realistic CDM parameter combination is able to account for the claimed feature near k = 0.1 h/ Mpc in the APM power spectrum, or the excess power at 100 Mpc/h wavelengths quoted by several recent surveys. Thus baryonic oscillations are not predicted to dominate existing measurements of clustering. We examine several effects which may mask the features which are predicted, and conclude that future galaxy surveys may be able to detect the oscillatory features in the power spectrum provided baryons comprise more than 15% of the total density, but that it will be a technically challenging achievement.Comment: 16 pages, 13 Figures, to be published in MNRA
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