35,397 research outputs found

    A two component jet model for the X-ray afterglow flat segment in short GRB 051221A

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    In the double neutron star merger or neutron star-black hole merger model for short GRBs, the outflow launched might be mildly magnetized and neutron rich. The magnetized neutron-rich outflow will be accelerated by the magnetic and thermal pressure and may form a two component jet finally, as suggested by Vlahakis, Peng & K\"{o}nigl (2003). We show in this work that such a two component jet model could well reproduce the multi-wavelength afterglow lightcurves, in particular the X-ray flat segment, of short GRB 051221A. In this model, the central engine need not to be active much longer than the prompt γ\gamma-ray emission.Comment: 11 pages, 2 figure; Accepted for publication by ApJ

    Periodicities in the occurrence of aurora as indicators of solar variability

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    A compilation of records of the aurora observed in China from the Time of the Legends (2000 - 3000 B.C.) to the mid-18th century has been used to infer the frequencies and strengths of solar activity prior to modern times. A merging of this analysis with auroral and solar activity patterns during the last 200 years provides basically continuous information about solar activity during the last 2000 years. The results show periodicities in solar activity that contain average components with a long period (approx. 412 years), three middle periods (approx. 38 years, approx. 77 years, and approx. 130 years), and the well known short period (approx. 11 years)

    The second phase transition in the pyrochlore oxide Cd2Re2O7

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    Evidence for another phase transition at 120 K in the metallic pyrochlore oxide Cd2Re2O7, following the structural transition at 200 K and followed by the superconducting transition at 1.0 K, is given through resistivity, magnetoresistance, specific heat, and X-ray diffraction measurements. The results indicate unique successive structural and electronic transitions occurring in the pyrochlore compound, revealing an interesting interplay between the crystal and electronic structures on the itinerant electron system in the pyrochlore lattice

    Reputation: configuring the symmetrical and asymmetrical paths to architecture in a retail setting

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    Grounded in social identity and attribution theories, this study focuses on the effect of architecture and its components on reputation. The relationships conceptualised were evaluated using data collected from a survey of 489 online and offline UK retail consumers and employees. To accommodate the equifinality and complexity of these relationships, this study employs fuzzy set qualitative comparative analysis, predictive validity and fit validity chec

    The X-ray afterglow of GRB 081109A: clue to the wind bubble structure

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    We present the prompt BAT and afterglow XRT data of Swift-discovered GRB081109A up to ~ 5\times 10^5 sec after the trigger, and the early ground-based optical follow-ups. The temporal and spectral indices of the X-ray afterglow emission change remarkably. We interpret this as the GRB jet first traversing the freely expanding supersonic stellar wind of the progenitor with density varying as ρr2\rho \propto r^{-2}. Then after approximately 300 sec the jet traverses into a region of apparent constant density similar to that expected in the stalled-wind region of a stellar wind bubble or the interstellar medium (ISM). The optical afterglow data are generally consistent with such a scenario. Our best numerical model has a wind density parameter {A0.02A_{*} \sim 0.02, a density of the stalled wind n0.12cm3n\sim 0.12 {\rm cm}^{-3}, and a transition radius 4.5×1017 \sim 4.5 \times 10^{17} cm}. Such a transition radius is smaller than that predicted by numerical simulations of the stellar wind bubbles and may be due to a rapidly evolving wind of the progenitor close to the time of its core-collapse.Comment: 7 pages, 5 figures, 2 tables, MNRAS accepted for publicatio

    A generalization of heterochromatic graphs

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    In 2006, Suzuki, and Akbari & Alipour independently presented a necessary and sufficient condition for edge-colored graphs to have a heterochromatic spanning tree, where a heterochromatic spanning tree is a spanning tree whose edges have distinct colors. In this paper, we propose ff-chromatic graphs as a generalization of heterochromatic graphs. An edge-colored graph is ff-chromatic if each color cc appears on at most f(c)f(c) edges. We also present a necessary and sufficient condition for edge-colored graphs to have an ff-chromatic spanning forest with exactly mm components. Moreover, using this criterion, we show that a gg-chromatic graph GG of order nn with E(G)>(nm2)|E(G)|>\binom{n-m}{2} has an ff-chromatic spanning forest with exactly mm (1mn11 \le m \le n-1) components if g(c)E(G)nmf(c)g(c) \le \frac{|E(G)|}{n-m}f(c) for any color cc.Comment: 14 pages, 4 figure

    Temperature - pressure phase diagram of the superconducting iron pnictide LiFeP

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    Electrical-resistivity and magnetic-susceptibility measurements under hydrostatic pressure up to p = 2.75 GPa have been performed on superconducting LiFeP. A broad superconducting (SC) region exists in the temperature - pressure (T-p) phase diagram. No indications for a spin-density-wave transition have been found, but an enhanced resistivity coefficient at low pressures hints at the presence of magnetic fluctuations. Our results show that the superconducting state in LiFeP is more robust than in the isostructural and isoelectronic LiFeAs. We suggest that this finding is related to the nearly regular [FeP_4] tetrahedron in LiFeP.Comment: 4 pages, 4 figure

    Contribution of geometric design parameters to knee implant performance: Conflicting impact of conformity on kinematics and contact mechanics

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    Background: Articular geometry of knee implant has a competing impact on kinematics and contact mechanics of total knee arthroplasty (TKA) such that geometry with lower contact pressure will impose more constraints on knee kinematics. The geometric parameters that may cause this competing effect have not been well understood. This study aimed to quantify the underlying relationships between implant geometry as input and its performance metrics as output. Methods: Parametric dimensions of a fixed-bearing cruciate retaining implant were randomized to generate a number of perturbed implant geometries. Performance metrics (i.e., maximum contact pressure, anterior–posterior range of motion [A-P ROM] and internal–external range of motion [I-E ROM]) of each randomized design were calculated using finite element analysis. The relative contributions of individual geometric variables to the performance metrics were then determined in terms of sensitivity indices (SI). Results: The femoral and tibial distal or posterior radii and femoral frontal radius are the key parameters. In the sagittal plane, distal curvature of the femoral and tibial influenced both contact pressure, i.e., SI = 0.57; SI = 0.65, and A-P ROM, i.e., SI = 0.58; SI = 0.6, respectively. However, posterior curvature of the femoral and tibial implants had a smaller impact on the contact pressure, i.e., SI = 0.31; SI = 0.23 and a higher impact on the I-E ROM, i.e., SI = 0.72; SI = 0.58. It is noteworthy that in the frontal plane, frontal radius of the femoral implant impacted both contact pressure (SI = 0.38) and I-E ROM (SI = 0.35). Conclusion: Findings of this study highlighted how changes in the conformity of the femoral and tibial can impact the performance metrics
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