2,663 research outputs found

    Shear Viscosity in a Perturbative Quark-Gluon-Plasma

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    Among the key features of hot and dense QCD matter produced in ultra-relativistic heavy-ion collisions at RHIC is its very low shear viscosity, indicative of the properties of a near-ideal fluid, and a large opacity demonstrated by jet energy loss measurements. In this work, we utilize a microscopic transport model based on the Boltzmann equation with quark and gluon degrees of freedom and cross sections calculated from perturbative Quantum Chromodynamics to simulate an ideal Quark-Gluon-Plasma in full thermal and chemical equilibrium. We then use the Kubo formalism to calculate the shear viscosity to entropy density ratio of the medium as a function of temperature and system composition. One of our key results is that the shear viscosity over entropy-density ratio η/s\eta/s becomes invariant to the chemical composition of the system when plotted as a function of energy-density instead of temperature.Comment: 11 pages, 8 figures: version #2 contains some revisions and added references to clarify relationship to previously published wor

    Surveying the Inner Halo of the Galaxy with 2MASS-Selected Horizontal Branch Candidates

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    We use 2MASS photometry to select blue horizontal branch (BHB) candidates covering the sky |b|>15 deg. A 12.5<J<15.5 sample of BHB stars traces the thick disk and inner halo to d<9 kpc, with a density comparable to that of M giant stars. We base our sample selection strategy on the Century Survey Galactic Halo Project, a survey that provides a complete, spectroscopically-identified sample of blue stars to a similar depth as the 2MASS catalog. We show that a -0.20<(J-H)_0<0.10, -0.10<(H-K)_0<0.10 color-selected sample of stars is 65% complete for BHB stars, and is composed of 47% BHB stars. We apply this photometric selection to the full 2MASS catalog, and see no spatial overdensities of BHB candidates at high Galactic latitude |b|>50 deg. We insert simulated star streams into the data and conclude that the high Galactic latitude BHB candidates are consistent with having no ~5 deg wide star stream with density greater than 0.33 objects deg^-2 at the 95% confidence level. The absence of structure suggests there have been no major accretion events in the inner halo in the last few Gyr. However, at low Galactic latitudes a two-point angular correlation analysis reveals structure on angular scales <1 deg. This structure is apparently associated with stars in the thick disk, and has a physical scale of 10-100 pc. Interestingly, such structures are expected by cosmological simulations that predict the majority of the thick disk may arise from accretion and disruption of satellite mergers.Comment: 11 pages, including figures. Accepted by AJ with minor revision

    Femto-Photography of Protons to Nuclei with Deeply Virtual Compton Scattering

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    Developments in deeply virtual Compton scattering allow the direct measurements of scattering amplitudes for exchange of a highly virtual photon with fine spatial resolution. Real-space images of the target can be obtained from this information. Spatial resolution is determined by the momentum transfer rather than the wavelength of the detected photon. Quantum photographs of the proton, nuclei, and other elementary particles with resolution on the scale of a fraction of a femtometer is feasible with existing experimental technology.Comment: To be published in Physical Review D. Replaces previous version with minor changes in presentatio

    Degenerate dispersive equations arising in the study of magma dynamics

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    An outstanding problem in Earth science is understanding the method of transport of magma in the Earth's mantle. Models for this process, transport in a viscously deformable porous media, give rise to scalar degenerate, dispersive, nonlinear wave equations. We establish a general local well-posedness for a physical class of data (roughly H1H^1) via fixed point methods. The strategy requires positive lower bounds on the solution. This is extended to global existence for a subset of possible nonlinearities by making use of certain conservation laws associated with the equations. Furthermore, we construct a Lyapunov energy functional, which is locally convex about the uniform state, and prove (global in time) nonlinear dynamic stability of the uniform state for any choice of nonlinearity. We compare the dynamics to that of other problems and discuss open questions concerning a larger range of nonlinearities, for which we conjecture global existence.Comment: 27 Pages, 7 figures are not present in this version. See http://www.columbia.edu/~grs2103/ for a PDF with figures. Submitted to Nonlinearit

    Suction rectal biopsy in the diagnosis of Hirschsprung's disease and chronic constipation

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    Suction rectal biopsy has gained increased acceptance as the means of definitively diagnosing Hirschsprung's disease as well as excluding this diagnosis when evaluating the child with chronic constipation. During the 11-year period from 1 July 1974 through 30 June 1985 at the University of Michigan, Mott Children's Hospital, 309 suction rectal biopsy specimens were evaluated. Of these, 293 were done for the evaluation of chronic constipation and/or Hirschsprung's disease. The remaining 16 were performed as a part of the work-up in patients with neuromuscular, glycogen storage, inflammatory bowel, or other diseases. Forty-two (14%) of the 293 patients were diagnosed as having Hirschsprung's disease at an average age of 14.4 months. This diagnosis was ruled out in the remaining 251 patients, whose age at biopsy averaged 2.7 years. There was one false-negative reading representing an incidence of 0.3%, with no false-positives. There were no complications. The suction rectal biopsy is a bedside or clinic procedure that reliably provides pathologic material adequate for the accurate diagnosis or exclusion of Hirschsprung's disease and offers a number of advantages over manometric, radiographic, histochemical, and open, full-thickness biopsy techniques.Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/47146/1/383_2004_Article_BF00166866.pd

    Orbit structure and (reversing) symmetries of toral endomorphisms on rational lattices

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    We study various aspects of the dynamics induced by integer matrices on the invariant rational lattices of the torus in dimension 2 and greater. Firstly, we investigate the orbit structure when the toral endomorphism is not invertible on the lattice, characterising the pretails of eventually periodic orbits. Next we study the nature of the symmetries and reversing symmetries of toral automorphisms on a given lattice, which has particular relevance to (quantum) cat maps.Comment: 29 pages, 3 figure
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