8,200 research outputs found

    Health care productivity.

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    An Emergentist Account of Collective Cognition in Collaborative Problem Solving

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    As a first step toward an emergentist theory of collective cognition in collaborative problem solving, we present a proto-theoretical account of how one might conceive and model the intersubjective processes that organize collective cognition into one or another--convergent, divergent, or tensive--cognitive regime. To explore the sufficiency of our emergentist proposal we instantiate a minimalist model of intersubjective convergence and simulate the tuning of collective cognition using data from an empirical study of small-group, collaborative problem solving. Using the results of this empirical simulation, we test a number of preliminary hypotheses with regard to patterns of interaction, how those patterns affect a cognitive regime, and how that cognitive regime affects the efficacy of a problem-solving group

    Public health and the sustainability of cities: Sydney airport's noise pollution and community wellbeing

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    The development of international airports is a driving force behind globalisation. But growth in air traffic is also a threat to sustainable community health in the vicinity of airports. Airports are an increasingly important dimension to the economic sustainability of cities but the health and wellbeing of its citizens must also be considered in the process of development assessment and impact mitigation

    Pneumoconiosis of Coal-Miners in Scotland

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    Abstract Not Provided

    Photochemistry

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    Photochemistry refers to the processes by which energy is transferred from electromagnetic radiation (in practice mainly ultraviolet and visible light) into chemical activity in gases, solid particles, and living matter. Photochemical processes partly control the initial conditions for the formation of stars and planets, they may leave traces of the early chemical evolution of planetary systems in the abundances of isotopes, they regulate the input of stellar energy into atmospheres of planets, and they play important roles in the chemistry of living organisms on Earth

    Detection of Interstellar C_2 and C_3 in the Small Magellanic Cloud

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    We report the detection of absorption from interstellar C_2 and C_3 toward the moderately reddened star Sk 143, located in the near 'wing' region of the SMC, in optical spectra obtained with the ESO VLT/UVES. These detections of C_2 (rotational levels J=0-8) and C_3 (J=0-12) absorption in the SMC are the first beyond our Galaxy. The total abundances of C_2 and C_3 (relative to H_2) are similar to those found in diffuse Galactic molecular clouds -- as previously found for CH and CN -- despite the significantly lower average metallicity of the SMC. Analysis of the rotational excitation of C_2 yields an estimated kinetic temperature T_k ~ 25 K and a moderately high total hydrogen density n_H ~ 870 cm^-3 -- compared to the T_01 ~ 45 K and n_H ~ 85-300 cm^-3 obtained from H_2. The populations of the lower rotational levels of C_3 are consistent with an excitation temperature of about 34 K.Comment: accepted to MNRAS; 10 pages, 6 figure

    Conference Summary

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    By any measure, IAU Symposium 280 has been an outstanding success: more than 400 participants represented at least 30 countries with 74 presentations and more than 300 posters. Beyond these numbers, it is evident that the cross-disciplinary field of astrochemistry is flourishing with excellent prospects for growth in the future. We have enjoyed the excitement of new, unexpected results from the Herschel Space Observatory and eagerly await new opportunities and facilities that will arise in the coming months and years
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