2,245 research outputs found

    Energy poverty: have we got the measure of it?

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    At the macro-level it has long been accepted that there is a strong relationship between energy and economic growth (IDS, 2003). In the 1990s, the development discourse began to focus on the effects that economic growth has had on poverty. However, an interest in the links between energy and poverty took more time to emerge2^2 Indeed, energy as an enabling factor in social transformations at the micro-level has not played a major role in the development discourse. Energy, unlike other infrastructure-related sectors such as water, transport and ICT, has also not been a central topic within the social sciences, including anthropology. The recent interest in climate change has focused on energy as the problem not part of the solution, particularly for the poor

    Companion Animal Demographics in the United States: A Historical Perspective

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    Modern American society recognizes the crucial role of data and information in evaluating and effectively addressing societal problems. Americans are bombarded with information on the economy, public health, social and psychological attitude trends, and other matters that are considered important. For example, no self-respecting politician would think of launching a political campaign or initiative without some sense of what the public might be worrying about. Addressing pet population issues should be no different. Data are needed in order to define the nature and scope of the dog and cat demographic challenge. Data can help people to understand the impact of “pet homelessness” on companion animals; to identify some of the characteristics of both successful and failed human-animal relationships; and to develop sound, effective, and long-lasting solutions that will strengthen humans’ relationships with companion animals and enhance companion animals’ welfare. Given the need for reliable data, what is known now about trends concerning the companion animal population and the shelters that help address the “homelessness” problem

    Adaptive Multidimensional Integration Based on Rank-1 Lattices

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    Quasi-Monte Carlo methods are used for numerically integrating multivariate functions. However, the error bounds for these methods typically rely on a priori knowledge of some semi-norm of the integrand, not on the sampled function values. In this article, we propose an error bound based on the discrete Fourier coefficients of the integrand. If these Fourier coefficients decay more quickly, the integrand has less fine scale structure, and the accuracy is higher. We focus on rank-1 lattices because they are a commonly used quasi-Monte Carlo design and because their algebraic structure facilitates an error analysis based on a Fourier decomposition of the integrand. This leads to a guaranteed adaptive cubature algorithm with computational cost O(mbm)O(mb^m), where bb is some fixed prime number and bmb^m is the number of data points

    Inflation and initial conditions in the pre-big bang scenario

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    The pre-big bang scenario describes the evolution of the Universe from an initial state approaching the flat, cold, empty, string perturbative vacuum. The choice of such an initial state is suggested by the present state of our Universe if we accept that the cosmological evolution is (at least partially) duality-symmetric. Recently, the initial conditions of the pre-big bang scenario have been criticized as they introduce large dimensionless parameters allowing the Universe to be "exponentially large from the very beginning". We agree that a set of initial parameters (such as the initial homogeneity scale, the initial entropy) larger than those determined by the initial horizon scale, H^{-1}, would be somewhat unnatural to start with. However, in the pre-big bang scenario, the initial parameters are all bounded by the size of the initial horizon. The basic question thus becomes: is a maximal homogeneity scale of order H^{-1} necessarily unnatural if the initial curvature is small and, consequently, H^{-1} is very large in Planck (or string) units? In the impossibility of experimental information one could exclude "a priori", for large horizons, the maximal homogeneity scale H^{-1} as a natural initial condition. In the pre-big bang scenario, however, pre-Planckian initial conditions are not necessarily washed out by inflation and are accessible (in principle) to observational tests, so that their naturalness could be also analyzed with a Bayesan approach, in terms of "a posteriori" probabilities.Comment: 4 pages, Latex, one figure. Many references added. The text has been improved in many points. To appear in Phys. Rev.

    Survey of Academic Field Experiences (SAFE): Trainees Report Harassment and Assault

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    Little is known about the climate of the scientific fieldwork setting as it relates to gendered experiences, sexual harassment, and sexual assault. We conducted an internet-based survey of field scientists (N = 666) to characterize these experiences. Codes of conduct and sexual harassment policies were not regularly encountered by respondents, while harassment and assault were commonly experienced by respondents during trainee career stages. Women trainees were the primary targets; their perpetrators were predominantly senior to them professionally within the research team. Male trainees were more often targeted by their peers at the research site. Few respondents were aware of mechanisms to report incidents; most who did report were unsatisfied with the outcome. These findings suggest that policies emphasizing safety, inclusivity, and collegiality have the potential to improve field experiences of a diversity of researchers, especially during early career stages. These include better awareness of mechanisms for direct and oblique reporting of harassment and assault and, the implementation of productive response mechanisms when such behaviors are reported. Principal investigators are particularly well positioned to influence workplace culture at their field sites
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