858 research outputs found

    Mesoscopic Effects in the Fractional Quantum Hall Regime: Chiral Luttinger versus Fermi Liquid

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    We study tunneling through an edge state formed around an antidot in the fractional quantum Hall regime using Wen's chiral Luttinger liquid theory extended to include mesoscopic effects. We identify a new regime where the Aharonov-Bohm oscillation amplitude exhibits a distinctive crossover from Luttinger liquid power-law behavior to Fermi-liquid-like behavior as the temperature is increased. Near the crossover temperature the amplitude has a pronounced maximum. This non-monotonic behavior and novel high-temperature nonlinear phenomena that we also predict provide new ways to distinguish experimentally between Luttinger and Fermi liquids.Comment: 13 pages, Revtex, Figure available from [email protected]

    A Morphology--Cosmology Connection for X--Ray Clusters

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    We employ N--body/3D3D gas dynamic simulations of the formation of galaxy clusters to determine whether cluster X--ray morphologies can be used as cosmological constraints. Confirming the analytic expectations of Richstone, Loeb, \& Turner, we demonstrate that cluster evolution is sensitive to the cosmological model in which the clusters form. We further show that evolutionary differences are echoed in the gross morphological features of the cluster X--ray emission. We examine current--epoch X--ray images of models originating from the same initial density fields evolved in three different cosmologies: (i) an unbiased, low density universe with \Omega_o \se 0.2; (ii) an unbiased universe dominated by vacuum energy with \Omega_o \se 0.2 and \lambda_o \se 0.8 and (iii) a biased Einstein--deSitter model (\Omega \se 1, σ8=0.59\sigma_8=0.59). Using measures of X--ray morphology such as the axial ratio and centroid shifting, we demonstrate that clusters evolved in the two low Ωo\Omega_o models are much more regular, spherically symmetric, and centrally condensed than clusters evolved in the Einstein--deSitter model. This morphology--cosmology connection, along with the availability of a large body of cluster X--ray observations, makes cluster X--ray morphology both a powerful and a practical cosmological discriminant.Comment: (uuencoded, compressed postscript, 9 pages including figures), CFA-370

    A Complete Spectroscopic Census of Abell 2029: A Tale of Three Histories

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    A rich spectroscopic census of members of the local massive cluster Abell 2029 includes 1215 members of A2029 and its two infalling groups, A2033 and a Southern Infalling Group (SIG). The two infalling groups are identified in spectroscopic, X-ray and weak lensing maps. We identify active galactic nuclei (AGN), star-forming galaxies, E+A galaxies, and quiescent galaxies based on the spectroscopy. The fractions of AGN and post-starburst E+A galaxies in A2029 are similar to those of other clusters. We derive the stellar mass (MM_{*})-metallicity of A2029 based on 227 star-forming members; A2029 members within 109M<M<109.5M10^{9} M_{\odot} < M _{*} < 10^{9.5} M_{\odot} are more metal rich than SDSS galaxies within the same mass range. We utilize the spectroscopic index Dn4000D_{n}4000, a strong age indicator, to trace past and future evolution of the A2029 system. The median Dn4000D_{n}4000 of the members decreases as the projected clustercentric distance increases for all three subsystems. The Dn4000MD_{n}4000 - M_{*} relations of the members in A2029 and its two infalling groups differ significantly indicating the importance of stochastic effects for understanding the evolution of cluster galaxy populations. In the main cluster, an excess around Dn40001.8D_{n}4000 \sim 1.8 indicates that some A2029 members became quiescent galaxies 2-3 Gyr ago consistent with the merger epoch of the X-ray sloshing pattern.Comment: 17 pages, 11 figures, submitted to Ap

    Applying Kolb\u27s Theory to Distance Learning

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    Recent advances in technology have brought major changes in pedagogy methods. Distance Learning (DL) has emerged as an innovative teaching method and it is becoming very popular in today’s education. We study a business simulation game in a DL environment and examine the learning outcomes and benefits of using the game in this environment. We also compare our test results to a game conducted in a traditional face-to-face class. Our findings show that students do not consider the DL teaching method to be worst than the traditional one. However, technical difficulties deterred the students to declare this method s superior. We conclude that further study of DL is necessary to: (1) realize its benefits; and (2) address the many challenges the creation of a DL learning environment poses

    Practice Parameter for the Assessment and Treatment of Children and Adolescents With Obsessive-Compulsive Disorder

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    Research in etiology, neurobiology, genetics, clinical correlates, and evidence-based treatments in children and adolescents with obsessive-compulsive disorder indicate a need for the revision of the Practice Parameters for the Assessment and Treatment of Children and Adolescents with Obsessive-Compulsive Disorder first published a decade ago. The present article highlights the clinical assessment and reviews and summarizes the evidence base for treatment. Based on this evidence, specific recommendations are provided for assessment, cognitive behavioral therapy, pharmacotherapy, combined treatment, and other interventions
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