2,665 research outputs found

    Non-gaussianity from the second-order cosmological perturbation

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    Several conserved and/or gauge invariant quantities described as the second-order curvature perturbation have been given in the literature. We revisit various scenarios for the generation of second-order non-gaussianity in the primordial curvature perturbation \zeta, employing for the first time a unified notation and focusing on the normalisation f_{NL} of the bispectrum. When the classical curvature perturbation first appears a few Hubble times after horizon exit, |f_{NL}| is much less than 1 and is, therefore, negligible. Thereafter \zeta (and hence f_{NL}) is conserved as long as the pressure is a unique function of energy density (adiabatic pressure). Non-adiabatic pressure comes presumably only from the effect of fields, other than the one pointing along the inflationary trajectory, which are light during inflation (`light non-inflaton fields'). During single-component inflation f_{NL} is constant, but multi-component inflation might generate |f_{NL}| \sim 1 or bigger. Preheating can affect f_{NL} only in atypical scenarios where it involves light non-inflaton fields. The curvaton scenario typically gives f_{NL} \ll -1 or f_{NL} = +5/4. The inhomogeneous reheating scenario can give a wide range of values for f_{NL}. Unless there is a detection, observation can eventually provide a limit |f_{NL}| \lsim 1, at which level it will be crucial to calculate the precise observational limit using second order theory.Comment: Latex file in Revtex style. 13 pages, 1 figure. v2: minor changes. Discussion in Subsection VI-A enlarged. References added. Conclusions unchanged. v3: minor typographic changes. Correlated and uncorrelated \chi^2 non-gaussianity concepts and consequences introduced. Section VI-A enlarged. Small change in Table I. References updated and added. Conclusions unchanged. Version to appear in Physical Review

    Fluorine gas as a cleaning agent for Apollo bulk-sample containers

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    A technique has been developed for cleaning Apollo bulk sample containers using fluorine gas as the cleaning agent

    Myself

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    Teaching controversial issues: Talking about religious freedom and the imagined ‘other’

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    Symposium: Teaching Controversial Issues Lee Jerome, Judy Pace, Helen Young, Sally Elton-Chalcraft and Anna Liddle The call to tackle controversial issues in citizenship, history, and other social studies disciplines increases as the world faces greater social, political, and economic crises (Kerr & Huddleston, 2015). Teachers’ ability to frame issues and their relevant content knowledge, utilize effective pedagogies, and create a supportive atmosphere is essential (Hahn, 1998). Controversial issues are "those problems and disputes that divide society and for which significant groups within society offer conflicting explanations and solutions based on alternative values" (Stradling et al., 1984, p. 2). They include public issues, related, for example, to terrorism, reproductive rights, and immigration (Hess, 2009), and sensitive questions related to contested histories (Foster, 2014) such as the partition of Ireland and culpability for genocide. Research shows that the discussion of controversial issues in an open classroom climate develops political knowledge and engagement (Hess & McAvoy, 2015) as well as tolerance (Avery, 2002). But teaching them successfully requires a particular set of knowledge, skills, and dispositions (Hess, 2009). Identifying an issue as controversial may be controversial itself (Camicia, 2008) and issues considered intensely controversial in some countries (e.g. gay marriage, collective health care) may be less so in others, and issues become more or less controversial over time (Hess, 2009). Therefore, teaching controversial issues often involves risk-taking (Kitson & McCully, 2005). Curricular resources and pedagogical structures can assist greatly, but school curriculum, culture, and policy can impede teachers’ efforts. In this symposium we share recent research that explores curricular, pedagogic, and policy implications of pursuing open explorations of controversial issues. Paper 1: Learning to teach controversial issues: Developmental and Contextual Factors How do preservice teachers learn to teach controversial issues in citizenship, social studies, and history? What factors support and constrain their risk-taking? This paper takes up Kitson & McCully’s (2005) continuum of risk-taking and reports findings from a study on preparing preservice teachers to teach controversial issues, conducted in Northern Ireland, England, and the United States. Out of 15 interviewed, 12 creatively used tools from their methods courses to teach lessons that made students explore different perspectives on an important issue. The novices practiced "contained risk-taking" (Author): They espoused social aims but only some taught to these aims. They used provocative resources but critical examination of them was minimal. They used dialogic pedagogies but sustained discussion was limited. Linkages between history and current concerns close to home were made in Northern Ireland but not in England. Factors that supported or constrained risk-taking included curriculum, timetables, students, mentor teachers, and school culture. The paper discusses implications for teacher education and school policy. Paper 2: Enabling young people to build their understanding of terrorism and extremism? A review of resources. This paper reviews the teaching resources on the Educate Against Hate website (DfE, on-line), which has been developed by the UK government ‘to provide practical advice, support and resources to protect children from extremism and radicalisation.’ The paper considers the resources in relation to research which has previously indicated what young people say they want and need (e.g. Jerome & Elwick, 2019), exploring their provenance; their adoption of counter-narratives; their levels of bias; their avoidance of issues; and their overall coherence. The paper concludes that the resources fall significantly short of young people’s expectations and often represent simplistic and uncritical counter-narratives. It argues that a genuinely educational approach will take more heed of young people’s opinions, and engage in a more critical exploration of the issues in order to support young people to build their understanding and make sense of their world post-9/11. Paper 3: Talking about religious freedom and the imagined ‘other’ This paper reports on student discussions in small groups and whole class plenaries related to religious freedom and toleration. We reflect on the ways in which students engaged with the stimulus material offered to them and illustrate how they often used their imagination to move significantly beyond the facts they were given. We argue this reflects a playful commitment to develop cognitive empathy and de-centre their discussions through forms of thought experiment, and that this therefore reflects the need to recognise the legitimate other in such debates. Our findings have implications for whether / how the fundamental British values should be taught more critically as controversial issues

    Model selection in cosmology

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    Model selection aims to determine which theoretical models are most plausible given some data, without necessarily considering preferred values of model parameters. A common model selection question is to ask when new data require introduction of an additional parameter, describing a newly discovered physical effect. We review model selection statistics, then focus on the Bayesian evidence, which implements Bayesian analysis at the level of models rather than parameters. We describe our CosmoNest code, the first computationally efficient implementation of Bayesian model selection in a cosmological context. We apply it to recent WMAP satellite data, examining the need for a perturbation spectral index differing from the scaleinvariant (Harrison–Zel'dovich) case

    Stochastic approaches to inflation model building

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    While inflation gives an appealing explanation of observed cosmological data, there are a wide range of different inflation models, providing differing predictions for the initial perturbations. Typically models are motivated either by fundamental physics considerations or by simplicity. An alternative is to generate large numbers of models via a random generation process, such as the flow equations approach. The flow equations approach is known to predict a definite structure to the observational predictions. In this paper, we first demonstrate a more efficient implementation of the flow equations exploiting an analytic solution found by Liddle (2003). We then consider alternative stochastic methods of generating large numbers of inflation models, with the aim of testing whether the structures generated by the flow equations are robust. We find that while typically there remains some concentration of points in the observable plane under the different methods, there is significant variation in the predictions amongst the methods considered.Comment: 7 pages RevTeX4 with 7 figures. Updated to match version accepted by PRD. Calculations extended to sixth-order and extra clarifications adde
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