5,619 research outputs found

    The White Witch of Rosehall

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    This project is made possible with funding by the Government of Ontario and through eCampusOntario’s support of the Virtual Learning Strategy.The White Witch of Rosehall (1929) is a legendary story by Jamaican author H. G. de Lisser. It tells the story of a haunting in Montego Bay, Jamaica where, according to the legend, the spirit of Annie Palmer haunts the grounds of Rose Hall plantation house

    A kiss in the dark

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    https://digitalcommons.ithaca.edu/sheetmusic/1084/thumbnail.jp

    A Dream Of Orange Blossoms : Kitty and Men

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    https://digitalcommons.library.umaine.edu/mmb-vp/3867/thumbnail.jp

    The Lonely Nest : Kitty

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    https://digitalcommons.library.umaine.edu/mmb-vp/5900/thumbnail.jp

    BONNSAI: a Bayesian tool for comparing stars with stellar evolution models

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    Powerful telescopes equipped with multi-fibre or integral field spectrographs combined with detailed models of stellar atmospheres and automated fitting techniques allow for the analysis of large number of stars. These datasets contain a wealth of information that require new analysis techniques to bridge the gap between observations and stellar evolution models. To that end, we develop BONNSAI (BONN Stellar Astrophysics Interface), a Bayesian statistical method, that is capable of comparing all available observables simultaneously to stellar models while taking observed uncertainties and prior knowledge such as initial mass functions and distributions of stellar rotational velocities into account. BONNSAI can be used to (1) determine probability distributions of fundamental stellar parameters such as initial masses and stellar ages from complex datasets, (2) predict stellar parameters that were not yet observationally determined and (3) test stellar models to further advance our understanding of stellar evolution. An important aspect of BONNSAI is that it singles out stars that cannot be reproduced by stellar models through χ2\chi^{2} hypothesis tests and posterior predictive checks. BONNSAI can be used with any set of stellar models and currently supports massive main-sequence single star models of Milky Way and Large and Small Magellanic Cloud composition. We apply our new method to mock stars to demonstrate its functionality and capabilities. In a first application, we use BONNSAI to test the stellar models of Brott et al. (2011a) by comparing the stellar ages inferred for the primary and secondary stars of eclipsing Milky Way binaries. Ages are determined from dynamical masses and radii that are known to better than 3%. We find that the stellar models reproduce the Milky Way binaries well. BONNSAI is available through a web-interface at http://www.astro.uni-bonn.de/stars/bonnsai.Comment: Accepted for publication in A&A; 15 pages, 10 figures, 4 tables; BONNSAI is available through a web-interface at http://www.astro.uni-bonn.de/stars/bonnsa

    Evaluating the Temporal Coherence of Archived Pages

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    PDF of a powerpoint presentation from the International Internet Preservation Consortium (IIPC) 2015 Conference at Stanford University, April 28, 2015. Also available on Slideshare.https://digitalcommons.odu.edu/computerscience_presentations/1004/thumbnail.jp

    On the consistent solution of the gap--equation for spontaneously broken λΦ4\lambda \Phi^4-theory

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    We present a self--consistent solution of the finite temperature gap--equation for λΦ4\lambda \Phi^4 theory beyond the Hartree-Fock approximation using a composite operator effective action. We find that in a spontaneously broken theory not only the so--called daisy and superdaisy graphs contribute to the resummed mass, but also resummed non--local diagrams are of the same order, thus altering the effective mass for small values of the latter.Comment: 15 pages of revtex + 3 uuencoded postscript figures, ENSLAPP A-488/9

    A classical explanation of quantization

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    In the context of our recently developed emergent quantum mechanics, and, in particular, based on an assumed sub-quantum thermodynamics, the necessity of energy quantization as originally postulated by Max Planck is explained by means of purely classical physics. Moreover, under the same premises, also the energy spectrum of the quantum mechanical harmonic oscillator is derived. Essentially, Planck's constant h is shown to be indicative of a particle's "zitterbewegung" and thus of a fundamental angular momentum. The latter is identified with quantum mechanical spin, a residue of which is thus present even in the non-relativistic Schroedinger theory.Comment: 20 pages; version accepted for publication in Foundations of Physic

    Expert chess memory: Revisiting the chunking hypothesis

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    After reviewing the relevant theory on chess expertise, this paper re-examines experimentally the finding of Chase and Simon (1973a) that the differences in ability of chess players at different skill levels to copy and to recall positions are attributable to the experts' storage of thousands of chunks (patterned clusters of pieces) in long-term memory. Despite important differences in the experimental apparatus, the data of the present experiments regarding latencies and chess relations between successively placed pieces are highly correlated with those of Chase and Simon. We conclude that the 2-second inter-chunk interval used to define chunk boundaries is robust, and that chunks have psychological reality. We discuss the possible reasons why Masters in our new study used substantially larger chunks than the Master of the 1973 study, and extend the chunking theory to take account of the evidence for large retrieval structures (templates) in long-term memory
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