11,918 research outputs found

    The Feeling of Being Ok

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    The Feeling of Being OK is an exhibition of appropriated imagery from unknown abandoned collections. Using the tension found in the enigmatic aspects of these materials, I investigate the fragility of the photograph and its capacity to fabricate memory and narrative. Designed to be a meditation on William Faulkner’s 1930 novel As I Lay Dying, this series focuses on themes including empathy and indifference, instability of identity, and life’s inevitable fate. By incorporating found materials such as vernacular objects and text into the installation, the potential for meaning is broadened. The work is installed in constellations or vignettes, allowing for metaphorical and poetic readings of the newly recontextualized material

    Gravitational radiation from the r-mode instability

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    The instability in the r-modes of rotating neutron stars can (in principle) emit substantial amounts of gravitational radiation (GR) which might be detectable by LIGO and similar detectors. Estimates are given here of the detectability of this GR based the non-linear simulations of the r-mode instability by Lindblom, Tohline and Vallisneri. The burst of GR produced by the instability in the rapidly rotating 1.4 solar mass neutron star in this simulation is fairly monochromatic with frequency near 960 Hz and duration about 100 s. A simple analytical expression is derived here for the optimal S/N for detecting the GR from this type of source. For an object located at a distance of 20 Mpc we estimate the optimal S/N to be in the range 1.2 to about 12.0 depending on the LIGO II configuration.Comment: 8 pages, 4 figure

    Favorite Folders: A Configurable, Scalable File Browser

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    Microsoft Windows Explorer, the most widely used file browser in Microsoft Windows, shows almost all directories in the file system. However, most users usually access only a subset of the directories in their machine. If the file browser shows only the directories users are interested in, they can select the directory they want more easily and quickly. This paper introduces a configurable, scalable file system explorer that reduces selection time by showing only the directories users want to see. We give users an easy way to hide directories behind a special ellipsis node. In addition, those hidden directories are one click away. We present a preliminary field study conducted to validate the concept of Favorite Folders and a theoretical model to predict the performance times. Keywords: Windows Explorer, file browser, adaptive interfaces, customizable interfaces UMIACS-TR-2003-38 HCIL-TR-2003-1

    Scaling of Reaction Zones in the A+B->0 Diffusion-Limited Reaction

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    We study reaction zones in three different versions of the A+B->0 system. For a steady state formed by opposing currents of A and B particles we derive scaling behavior via renormalization group analysis. By use of a previously developed analogy, these results are extended to the time-dependent case of an initially segregated system. We also consider an initially mixed system, which forms reaction zones for dimension d<4. In this case an extension of the steady-state analogy gives scaling results characterized by new exponents.Comment: 4 pages, REVTeX 3.0 with epsf, 2 uuencoded postscript figures appended, OUTP-94-33

    Effect of hyperon bulk viscosity on neutron-star r-modes

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    Neutron stars are expected to contain a significant number of hyperons in addition to protons and neutrons in the highest density portions of their cores. Following the work of Jones, we calculate the coefficient of bulk viscosity due to nonleptonic weak interactions involving hyperons in neutron-star cores, including new relativistic and superfluid effects. We evaluate the influence of this new bulk viscosity on the gravitational radiation driven instability in the r-modes. We find that the instability is completely suppressed in stars with cores cooler than a few times 10^9 K, but that stars rotating more rapidly than 10-30% of maximum are unstable for temperatures around 10^10 K. Since neutron-star cores are expected to cool to a few times 10^9 K within seconds (much shorter than the r-mode instability growth time) due to direct Urca processes, we conclude that the gravitational radiation instability will be suppressed in young neutron stars before it can significantly change the angular momentum of the star.Comment: final PRD version, minor typos etc correcte

    Optimal combinations of imperfect objects

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    We address the question of how to make best use of imperfect objects, such as defective analog and digital components. We show that perfect, or near-perfect, devices can be constructed by taking combinations of such defects. Any remaining objects can be recycled efficiently. In addition to its practical applications, our `defect combination problem' provides a novel generalization of classical optimization problems.Comment: 4 pages, 3 figures, minor change

    Model-based asymptotically optimal dispersion measure correction for pulsar timing

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    In order to reach the sensitivity required to detect gravitational waves, pulsar timing array experiments need to mitigate as much noise as possible in timing data. A dominant amount of noise is likely due to variations in the dispersion measure. To correct for such variations, we develop a statistical method inspired by the maximum likelihood estimator and optimal filtering. Our method consists of two major steps. First, the spectral index and amplitude of dispersion measure variations are measured via a time-domain spectral analysis. Second, the linear optimal filter is constructed based on the model parameters found in the first step, and is used to extract the dispersion measure variation waveforms. Compared to current existing methods, this method has better time resolution for the study of short timescale dispersion variations, and generally produces smaller errors in waveform estimations. This method can process irregularly sampled data without any interpolation because of its time-domain nature. Furthermore, it offers the possibility to interpolate or extrapolate the waveform estimation to regions where no data is available. Examples using simulated data sets are included for demonstration.Comment: 15 pages, 15 figures, submitted 15th Sept. 2013, accepted 2nd April 2014 by MNRAS. MNRAS, 201

    Parity Problem With A Cellular Automaton Solution

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    The parity of a bit string of length NN is a global quantity that can be efficiently compute using a global counter in O(N){O} (N) time. But is it possible to find the parity using cellular automata with a set of local rule tables without using any global counter? Here, we report a way to solve this problem using a number of r=1r=1 binary, uniform, parallel and deterministic cellular automata applied in succession for a total of O(N2){O} (N^2) time.Comment: Revtex, 4 pages, final version accepted by Phys.Rev.

    Renormalization Group Study of the A+B->0 Diffusion-Limited Reaction

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    The A+B→0A + B\to 0 diffusion-limited reaction, with equal initial densities a(0)=b(0)=n0a(0) = b(0) = n_0, is studied by means of a field-theoretic renormalization group formulation of the problem. For dimension d>2d > 2 an effective theory is derived, from which the density and correlation functions can be calculated. We find the density decays in time as a,b \sim C\sqrt{\D}(Dt)^{-d/4} for d<4d < 4, with \D = n_0-C^\prime n_0^{d/2} + \dots, where CC is a universal constant, and Câ€ČC^\prime is non-universal. The calculation is extended to the case of unequal diffusion constants DA≠DBD_A \neq D_B, resulting in a new amplitude but the same exponent. For d≀2d \le 2 a controlled calculation is not possible, but a heuristic argument is presented that the results above give at least the leading term in an Ï”=2−d\epsilon = 2-d expansion. Finally, we address reaction zones formed in the steady-state by opposing currents of AA and BB particles, and derive scaling properties.Comment: 17 pages, REVTeX, 13 compressed figures, included with epsf. Eq. (6.12) corrected, and a moderate rewriting of the introduction. Accepted for publication in J. Stat. Phy
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