1,022 research outputs found

    Content-Based Video Retrieval in Historical Collections of the German Broadcasting Archive

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    The German Broadcasting Archive (DRA) maintains the cultural heritage of radio and television broadcasts of the former German Democratic Republic (GDR). The uniqueness and importance of the video material stimulates a large scientific interest in the video content. In this paper, we present an automatic video analysis and retrieval system for searching in historical collections of GDR television recordings. It consists of video analysis algorithms for shot boundary detection, concept classification, person recognition, text recognition and similarity search. The performance of the system is evaluated from a technical and an archival perspective on 2,500 hours of GDR television recordings.Comment: TPDL 2016, Hannover, Germany. Final version is available at Springer via DO

    It's OK not to be OK: Shared Reflections from two PhD Parents in a Time of Pandemic

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    Adopting an intersectional feminist lens, we explore our identities as single and co‐parents thrust into the new reality of the UK COVID‐19 lockdown. As two PhD students, we present shared reflections on our intersectional and divergent experiences of parenting and our attempts to protect our work and families during a pandemic. We reflect on the social constructions of ‘masculinities’ and ‘emphasized femininities’ as complicated influence on our roles as parents. Finally, we highlight the importance of time and self‐care as ways of managing our shared realities during this uncertain period. Through sharing reflections, we became closer friends in mutual appreciation and solidarity as we learned about each other’s struggles and vulnerabilities

    Immigrant populations, work and health—a systematic literature review

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    Objectives This paper summarizes the information on immigrant occupational health available from recent studies, incorporating varied study designs. Methods A systematic search was carried out in PubMed employing terms of interest to the study and related terms supplied by the same search engine. Articles were selected through the following process: (i) reading the title and abstract, in English or Spanish, for the period 1990–2005, (ii) reading of the entire text of selected articles; (iii) making a manual search of the relevant citations in the selected articles; (iv) eliminating articles without a focus on the themes of central interest (immigration, work, and health), and (v) reading and analyzing the definitive article set. No quality criteria were used in the article selection. Results The location of studies was not straightforward and required careful thought about the search terms. The included 48 papers were often multifaceted and difficult to categorize. They generally came from countries historically associated with immigration and described occupational risk factors, health consequences, and the social, economic, and cultural influences on worker health. They were also based on data, surveillance, training, and preventive measures that were inadequate. Conclusions Increased migration is a reality in industrialized countries all over the world, and it has social, political, and economic consequences for migrating groups, as well as for their sending and host societies. More reliable data, targeted appropriate interventions, and enforcement of existing regulations are necessary to improve the health of immigrant workers. Furthermore, studies in sending and developing countries should be encouraged to form a more complete understanding of this complex situation

    Development of the electroweak phase transition and baryogenesis

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    We investigate the evolution of the electroweak phase transition, using a one-Higgs effective potential that can be regarded as an approximation for the Minimal Supersymmetric Standard Model. The phase transition occurs in a small interval around a temperature T_t below the critical one. We calculate this temperature as a function of the parameters of the potential and of a damping coefficient related to the viscosity of the plasma. The parameters that are relevant for baryogenesis, such as the velocity and thickness of the walls of bubbles and the value of the Higgs field inside them, change significantly in the range of temperatures where the first-order phase transition can occur. However, we find that in the likely interval for T_t there is no significant variation of these parameters. Furthermore, the temperature T_t is in general not far below the temperature at which bubbles begin to nucleate.Comment: 26 pages, 7 figures; typos corrected, reference adde

    Strong Coupling Corrections to the Ginzburg-Landau Theory of Superfluid ^{3}He

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    In the Ginzburg-Landau theory of superfluid 3^{3}He, the free energy is expressed as an expansion of invariants of a complex order parameter. Strong coupling effects, which increase with increasing pressure, are embodied in the set of coefficients of these order parameter invariants\cite{Leg75,Thu87}. Experiments can be used to determine four independent combinations of the coefficients of the five fourth order invariants. This leaves the phenomenological description of the thermodynamics near TcT_{c} incomplete. Theoretical understanding of these coefficients is also quite limited. We analyze our measurements of the magnetic susceptibility and the NMR frequency shift in the BB-phase which refine the four experimental inputs to the phenomenological theory. We propose a model based on existing experiments, combined with calculations by Sauls and Serene\cite{Sau81} of the pressure dependence of these coefficients, in order to determine all five fourth order terms. This model leads us to a better understanding of the thermodynamics of superfluid 3^{3}He in its various states. We discuss the surface tension of bulk superfluid 3^{3}He and predictions for novel states of the superfluid such as those that are stabilized by elastic scattering of quasiparticles from a highly porous silica aerogel.Comment: 9 pages, 7 figures, 2 table

    Transport coefficients in the early universe

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    We calculate numerically the electrical conductivity σ\sigma, heat conductivity Îș\kappa and shear viscosity η\eta of the hot plasma present in the early universe for the temperature interval 1\MeV\lsim T\lsim 10\GeV. We use the Boltzmann collision equation to compute all the scattering matrix elements and regulate them by the thermal masses of the tt- and uu-channel particles. No leading order approximation is needed because of the numerical integration routines used.Comment: LaTeX, 24 pages, 7 ps figure

    Cosmological Magnetic Fields from Primordial Helical Seeds

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    Most early Universe scenarios predict negligible magnetic fields on cosmological scales if they are unprocessed during subsequent expansion of the Universe. We present a new numerical treatment of the evolution of primordial fields and apply it to weakly helical seeds as they occur in certain early Universe scenarios. We find that initial helicities not much larger than the baryon to photon number can lead to fields of about 10^{-13} Gauss with coherence scales slightly below a kilo-parsec today.Comment: 4 revtex pages, 2 postscript figures include

    Constraints on the Electrical Charge Asymmetry of the Universe

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    We use the isotropy of the Cosmic Microwave Background to place stringent constraints on a possible electrical charge asymmetry of the universe. We find the excess charge per baryon to be qe−p<10−26eq_{e-p}<10^{-26}e in the case of a uniform distribution of charge, where ee is the charge of the electron. If the charge asymmetry is inhomogeneous, the constraints will depend on the spectral index, nn, of the induced magnetic field and range from qe−p<5×10−20eq_{e-p}<5\times 10^{-20}e (n=−2n=-2) to qe−p<2×10−26eq_{e-p}<2\times 10^{-26}e (n≄2n\geq 2). If one could further assume that the charge asymmetries of individual particle species are not anti-correlated so as to cancel, this would imply, for photons, qÎł<10−35eq_\gamma< 10^{-35}e; for neutrinos, qÎœ<4×10−35eq_\nu<4\times10^{-35}e; and for heavy (light) dark matter particles qdm<4×10−24eq_{\rm dm}<4\times10^{-24}e (qdm<4×10−30eq_{\rm dm}<4\times10^{-30}e).Comment: New version to appear in JCA

    Entanglement-Enhanced Quantum Key Distribution

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    We present and analyze a quantum key distribution protocol based on sending entangled N-qubit states instead of single-qubit ones as in the trail-blazing scheme by Bennett and Brassard (BB84). Since the qubits are sent individually, an eavesdropper is limited to accessing them one by one. In an intercept-resend attack, this fundamental restriction allows one to make the eavesdropper's information on the transmitted key vanish if even one of the qubits is not intercepted. The implied upper bound 1/(2N) for Eve's information is further shown not to be the lowest since in the case N = 2, the information can be reduced to less than 30% of that in BB84. In general, the protocol is at least as secure as BB84.Comment: 7 pages, 5 figures, new result

    Magnetic Fields from Phase Transitions

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    The generation of primordial magnetic fields from cosmological phase transitions is discussed, paying particular attention to the electroweak transition and to the various definitions of the `average' field that have been put forward. It is emphasised that only the volume average has dynamical significance as a seed for galactic dynamos. On rather general grounds of causality and energy conservation, it is shown that, in the absence of MHD effects that transfer power in the magnetic field from small to large scales, processes occurring at the electroweak transition cannot generate fields stronger than 10−2010^{-20} Gauss on a scale of 0.5 Mpc. However, it is implausible that this upper bound could ever be reached, as it would require all the energy in the Universe to be turned into a magnetic field coherent at the horizon scale. Non-linear MHD effects seem therefore to be necessary if the electroweak transition is to create a primordial seed field.Comment: 6pp RevTeX. Correct finished version supplie
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