21,564 research outputs found

    Mill and Pettit on Freedom, Domination, and Freedom-as-Domination

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    Pettit endorses a ‘republican’ conception of social freedom of the person as consisting of a state of non-domination, and takes this to refute Mill’s ‘liberal’ claim that non-domineering but coercive interference can compromise social freedom of choice. This paper argues that Pettit’s interpretation is true to the extent that Mill believes that the legitimate, non-arbitrary and just coercion of would-be dominators, for the sake of preventing them from dominating others, can render them unfree to choose to do so without rendering them socially unfree (qua dominated) persons in their own right. However, contra Pettit, Mill is correct to reject the ‘republican’ view for at least two reasons. Firstly, it enables him to avoid commitment to the implausible implication that would-be dominators who sincerely deny any interest in a shared system of basic liberties are automatically rendered unfree persons by the coercion necessary to uphold such a system. Secondly, it enables him to avoid begging the question against ‘immoralists’ like Nietzsche, whose opposition to systems of reciprocal non-domination is at least partly motivated by the losses of social freedom of choice they entail for those they deem to be worthy of dominating others

    ABC for Temporally Sampled Genetic Data

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    ABC for Temporally Sampled Genetic Dat

    Statement of Richard A. Beaumont Before the Commission on the Future of Worker-Management Relations

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    Testimony_Beaumont_011994.pdf: 483 downloads, before Oct. 1, 2020

    Linear and nonlinear interactions between the earth tide and a tectonically stressed earth

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    In the vincinity of earthquake focal regions, conditions may not be equal. Crustal rocks stressed to more than approximately 0.6 of their failure strength exhibit material properties over and above that of linear elasticity. Interactions between the earth tide and crustal rocks that are under high tectonic stress are discussed in terms of simple phenomenological models. In particular, the difference between a nonlinear elastic model of dilatancy and a dilatancy model that exhibits hysteresis is noted. It is concluded that the small changes in stress produced by the earth tide act as a probe of the properties of crustal rocks. Observations of earth tide tilts and strains in such high stress zones may, therefore, provide keys to the constitutive properties and the tectonic stress rate tensor of these zones

    Optimisation of work flow

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    AeroSpace Technologies of Australia (ASTA) is a supplier of aircraft components for several of the world's major aircraft manufacturers. Its anticipation of a substantial increase in demand has led to concern as to its ability to satisfy customer imposed schedules. ASTA's main concern is scheduling at its five autoclaves. The autoclaves, which are large pressurised ovens in which components are cured before non destructive testing and final assembly, appear to be the bottlenecks in ASTA's manufacturing process. ASTA came to the Australian Mathematics-in-Industry Study Group (MISG) with the objective of developing an optimised loading plan for the autoclaves to improve their utilisation while meeting demand for final components. This report discusses the results of an intensive three day study by the MISG group working on the ASTA problem. Its findings were that: • Modifying the way in which Materials Requirements Planning (MRP) is used may usefully increase autoclave utilisation. • A single product which will account for 60% of factory hours could and should be scheduled separately. • It is feasible and very helpful to group products into a small number of sets with common autoclave processing requirements. • Integer programming models modelling the production line show considerable promise and should be developed further

    Take care of yourself

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    This article focuses on how compassion focused techniques that encourage self-reflection can help student practitioners to promote self-car

    Building an Optimal Census of the Solar Neighborhood with Pan-STARRS Data

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    We estimate the fidelity of solar neighborhood (D < 100 pc) catalogs soon to be derived from Pan-STARRS astrometric data. We explore two quantities used to measure catalog quality: completeness, the fraction of desired sources included in a catalog; and reliability, the fraction of entries corresponding to desired sources. We show that the main challenge in identifying nearby objects with Pan-STARRS will be reliably distinguishing these objects from distant stars, which are vastly more numerous. We explore how joint cuts on proper motion and parallax will impact catalog reliability and completeness. Using synthesized astrometry catalogs, we derive optimum parallax and proper motion cuts to build a census of the solar neighborhood with the Pan-STARRS 3 Pi Survey. Depending on the Galactic latitude, a parallax cut pi / sigma pi > 5 combined with a proper motion cut ranging from mu / sigma mu > 1-8 achieves 99% reliability and 60% completeness.Comment: 7 Pages, 4 Figures, 3 Tables. PASP in pres

    Discerning the Form of the Dense Core Mass Function

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    We investigate the ability to discern between lognormal and powerlaw forms for the observed mass function of dense cores in star forming regions. After testing our fitting, goodness-of-fit, and model selection procedures on simulated data, we apply our analysis to 14 datasets from the literature. Whether the core mass function has a powerlaw tail or whether it follows a pure lognormal form cannot be distinguished from current data. From our simulations it is estimated that datasets from uniform surveys containing more than approximately 500 cores with a completeness limit below the peak of the mass distribution are needed to definitively discern between these two functional forms. We also conclude that the width of the core mass function may be more reliably estimated than the powerlaw index of the high mass tail and that the width may also be a more useful parameter in comparing with the stellar initial mass function to deduce the statistical evolution of dense cores into stars.Comment: 6 pages, 2 figures, accepted for publication in PAS
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