3,550 research outputs found

    Peripheral Meson Model of Deep Inelastic Rapidity Gap Events

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    We show that a peripheral meson model can explain the large deep inelastic electron-proton scattering rapidity gap events observed at HERA.Comment: 12 pages, 2 figure

    Do management practices matter in further education?

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    Further education and sixth form colleges are key institutions for facilitating skill acquisition among 16–19 year olds in the UK. They enrol half a school cohort after completion of their lower secondary education, and this includes a disproportionate number from low-income backgrounds. Yet little is known about what could improve performance in these institutions. We conduct the world's first management practices survey in such institutions, and match this to administrative longitudinal data on over 40,000 students. Value-added regressions with rich controls suggest that structured management matters for educational outcomes, especially for students from low-income backgrounds. For this group, in a hypothetical scenario where an individual is moved from a college at the 10th percentile of management practices to the 90th, this would be associated with 8% higher probability of achieving a good high school qualification, nearly half of the educational gap between those from poor and non-poor backgrounds. Hence improving management practices may be an important channel for reducing inequalities

    Cryptic disease-induced mortality may cause host extinction in an apparently stable host- parasite system

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    The decline of wildlife populations due to emerging infectious disease often shows a common pattern: the parasite invades a naive host population, producing epidemic disease and a population decline, sometimes with extirpation. Some susceptible host populations can survive the epidemic phase and persist with endemic parasitic infection. Understanding host–parasite dynamics leading to persistence of the system is imperative to adequately inform conservation practice. Here we combine field data, statistical and mathematical modelling to explore the dynamics of the apparently stable Rhinoderma darwinii–Batrachochytrium dendrobatidis (Bd) system. Our results indicate that Bd-induced population extirpation may occur even in the absence of epidemics and where parasite prevalence is relatively low. These empirical findings are consistent with previous theoretical predictions showing that highly pathogenic parasites are able to regulate host populations even at extremely low prevalence, highlighting that disease threats should be investigated as a cause of population declines even in the absence of an overt increase in mortality

    Circular waste management of electric vehicle batteries: legal and technical perspectives from the EU and the UK post Brexit

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    Copyright © 2021 The Authors. In light of the climate change, interdisciplinary solutions are needed to deal with end-of-life lithium-ion batteries (LIBs) that are used in Electric vehicles (EVs) in order to avoid a waste problem in the future. Building on both legal and technical perspectives, this paper criticises the current EU and UK frameworks and policies on batteries waste management which fail to address technological innovation, especially, in terms of the creation of a market for ‘second life’ of EV batteries which are subject to the electrochemical performance and durability and safety parameters, as well as LIB recycling in support of a circular economy. Most importantly, it also addresses recent developments in the EU in terms of a proposal for the EU new Batteries Regulation and the impact of Brexit in the UK for its future policy shape

    Disk Evolution in W5: Intermediate Mass Stars at 2-5 Myr

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    We present the results of a survey of young intermediate mass stars (age <<~5 Myr, 1.5 <M<M_{\star} \leq 15 MM_{\odot}) in the W5 massive star forming region. We use combined optical, near-infrared and {\it Spitzer} Space Telescope photometry and optical spectroscopy to define a sample of stars of spectral type A and B and examine their infrared excess properties. We find objects with infrared excesses characteristic of optically thick disks, i.e. Herbig AeBe stars. These stars are rare: <<1.5% of the entire spectroscopic sample of A and B stars, and absent among stars more massive than 2.4 MM_\odot. 7.5% of the A and B stars possess infrared excesses in a variety of morphologies that suggest their disks are in some transitional phase between an initial, optically thick accretion state and later evolutionary states. We identify four morphological classes based on the wavelength dependence of the observed excess emission above theoretical photospheric levels: (a) the optically thick disks; (b) disks with an optically thin excess over the wavelength range 2 to 24 \micron, similar to that shown by Classical Be stars; (c) disks that are optically thin in their inner regions based on their infrared excess at 2-8 \micron and optically thick in their outer regions based on the magnitude of the observed excess emission at 24 \micron; (d) disks that exhibit empty inner regions (no excess emission at λ\lambda \leq 8 \micron) and some measurable excess emission at 24 \micron. A sub-class of disks exhibit no significant excess emission at λ\lambda \leq 5.8 \micron, have excess emission only in the {\it Spitzer} 8 \micron band and no detection at 24 \micron. We discuss these spectral energy distribution (SED) types, suggest physical models for disks exhibiting these emission patterns and additional observations to test these theories.Comment: 35 pages, 10 figures, accepted to Astrophysical Journa
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