2,173 research outputs found

    Towards an improved understanding of eta --> gamma^* gamma^*

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    We argue that high-quality data on the reaction e+e−→π+π−ηe^+e^-\to \pi^+\pi^-\eta will allow one to determine the double off-shell form factor η→γ∗γ∗\eta \to \gamma^*\gamma^* in a model-independent way with controlled accuracy. This is an important step towards a reliable evaluation of the hadronic light-by-light scattering contribution to the anomalous magnetic moment of the muon. When analyzing the existing data for e+e−→π+π−ηe^+e^- \to \pi^+\pi^-\eta in the range of total energies 1GeV2<Q22<(4.5GeV)21\text{GeV}^2<Q_2^2<(4.5\text{GeV})^2, we demonstrate that the double off-shell form factor Fηγ∗γ∗(Q12,Q22)F_{\eta\gamma^*\gamma^*}(Q_1^2,Q_2^2) is consistent with the commonly employed factorization ansatz at least for Q12<1GeV2Q_1^2<1\text{GeV}^2, if the effect of the a2a_2 meson is taken into account. However, better data are needed to draw firm conclusions.Comment: 7 pages, 3 figure

    Bodies without names: A global challenge

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    The Clustering of Massive Halos

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    The clustering properties of dark matter halos are a firm prediction of modern theories of structure formation. We use two large volume, high-resolution N-body simulations to study how the correlation function of massive dark matter halos depends upon their mass and formation history. We find that halos with the lowest concentrations are presently more clustered than those of higher concentration, the size of the effect increasing with halo mass; this agrees with trends found in studies of lower mass halos. The clustering dependence on other characterizations of the full mass accretion history appears weaker than the effect with concentration. Using the integrated correlation function, marked correlation functions, and a power-law fit to the correlation function, we find evidence that halos which have recently undergone a major merger or a large mass gain have slightly enhanced clustering relative to a randomly chosen population with the same mass distribution.Comment: 10 pages, 8 figures; text improved, references and one figure added; accepted for publication in Ap

    Fungicide efficacy against botrytis cinerea at different positions on grape shoots

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    CITATION: Van Rooi, C. & Holz, G. 2003. Fungicide efficacy against botrytis cinerea at different positions on grape shoots. South African Journal of Enology & Viticulture, 24(1):11-15, doi:10.21548/24-1-2145.The original publication is available at http://www.journals.ac.za/index.php/sajevFungicide efficacy at different positions on grape shoots was determined on vinelets inoculated with Botrytis cinerea. To ensure proper fungicide coverage, vinelets (table grape cultivar Dauphine, wine grape cultivar Merlot noir), prepared from cuttings, were sprayed in a spray chamber at the recommended dosages with iprodione, pyrimethanil, cyprodinil/fludioxonil and fenhexamid. Vinelets for the control treatment were left unsprayed. After 24 h the vinelets were dusted with dry, airborne conidia in a settling ower to reduce the sporadic occurrence of the pathogen on shoots and incubated for 24 h at high relative humidity (±93 % ) to promote infection. Fungicide efficacy was determined by observing intact vinelets for symptom expression at nodes, internodes, leaf blades, petioles and inflorescences, and by determining surface colonisation (shoots left unsterile) and penetration (surfacedisinfested shoots) by isolation studies. Symptoms of B. cinerea decay did not develop on sprayed and unsprayed vinelets that were kept in dry chambers during the 2-week observation period. The pathogen, however, developed from the isolated parts. On the unsprayed vinelets for both cultivars B. cinerea incidences recorded on two media and the two sterility regimes were significantly higher on leaf blades than on the petioles, shoot pieces and inflorescences. The isolation studies showed that the different fungicides were highly and nearly equally efficient in reducing superficial B. cinerea and latent infection at the various positions. In the case of leaf blades B. cinerea incidence was significantly reduced by each fungicide on both cultivars. This was not the case for the other parts, which yielded B. cinerea at low incidences under the two sterility regimes. The study showed that the fungicides used in this study, if applied properly to shoots at the pre-bloom stage, should effectively reduce the amount of B. cinerea in leaves and completely prevent the infection of nodes, internodes and inflorescences.http://www.journals.ac.za/index.php/sajev/article/view/2145Publisher's versio

    Regge Calculus in Teleparallel Gravity

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    In the context of the teleparallel equivalent of general relativity, the Weitzenbock manifold is considered as the limit of a suitable sequence of discrete lattices composed of an increasing number of smaller an smaller simplices, where the interior of each simplex (Delaunay lattice) is assumed to be flat. The link lengths between any pair of vertices serve as independent variables, so that torsion turns out to be localized in the two dimensional hypersurfaces (dislocation triangle, or hinge) of the lattice. Assuming that a vector undergoes a dislocation in relation to its initial position as it is parallel transported along the perimeter of the dual lattice (Voronoi polygon), we obtain the discrete analogue of the teleparallel action, as well as the corresponding simplicial vacuum field equations.Comment: Latex, 10 pages, 2 eps figures, to appear in Class. Quant. Gra

    \u3csup\u3e1\u3c/sup\u3eH NMR Studies on the CuA Center of Nitrous Oxide Reductase from \u3cem\u3ePseudomonas stutzeri\u3c/em\u3e

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    1H NMR spectra of the CuA center of N2OR from Pseudomonas stutzeri, and a mutant enzyme that contains only CuA, were recorded in both H2O- and D2O-buffered solution at pH 7.5. Several sharp, well-resolved hyperfine-shifted 1H NMR signals were observed in the 60 to −10 ppm chemical shift range. Comparison of the native and mutant N2OR spectra recorded in H2O-buffered solutions indicated that several additional signals are present in the native protein spectrum. These signals are attributed to a dinuclear copper(II) center. At least two of the observed hyperfine-shifted signals associated with the dinuclear center, those at 23.0 and 13.2 ppm, are lost upon replacement of H2O buffer with D2O buffer. These data indicate that at least two histidine residues are ligands of a dinuclear Cu(II) center. Comparison of the mutant N2OR 1H NMR spectra recorded in H2O and D2O indicates that three signals, c (27.5 ppm), e (23.6 ppm), and i (12.4 ppm), are solvent exchangeable. The two most strongly downfield-shifted signals (c and e) are assigned to the two Nε2H (N-H) protons of the coordinated histidine residues, while the remaining exchangeable signal is assigned to a backbone N-H proton in close proximity to the CuA cluster. Signal e was found to decrease in intensity as the temperature was increased, indicating that proton e resides on a more solvent-exposed histidine residue. One-dimensional nOe studies at pH 7.5 allowed the histidine ring protons to be definitively assigned, while the remaining signals were assigned by comparison to previously reported spectra from CuA centers. The temperature dependence of the observed hyperfine-shifted 1H NMR signals of mutant N2OR were recorded over the temperature range of 276−315 K. Both Curie and anti-Curie temperature dependencies are observed for sets of hyperfine-shifted protons. Signals a and h (cysteine protons) follow anti-Curie behavior (contact shift increases with increasing temperatures), while signals b−g, i, and j (histidine protons) follow Curie behavior (contact shift decreases with increasing temperatures). Fits of the temperature dependence of the observed hyperfine-shifted signals provided the energy separation (ΔEL) between the ground (2B3u) and excited (2B2u) states. The temperature data obtained for all of the observed hyperfine-shifted histidine ligand protons provided a ΔEL value of 62 ± 35 cm-1. The temperature dependence of the observed cysteine CβH and CαH protons (a and h) were fit in a separate experiment providing a ΔEL value of 585 ± 125 cm-1. The differences between the ΔEL values determined by 1H NMR spectroscopy and those determined by EPR or MCD likely arise from coupling between relatively low-frequency vibrational states and the ground and excited electronic states

    Aharonov-Bohm Effect and Disclinations in an Elastic Medium

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    In this work we investigate quasiparticles in the background of defects in solids using the geometric theory of defects. We use the parallel transport matrix to study the Aharonov-Bohm effect in this background. For quasiparticles moving in this effective medium we demonstrate an effect similar to the gravitational Aharonov- Bohm effect. We analyze this effect in an elastic medium with one and NN defects.Comment: 6 pages, Revtex

    An Analysis of Rogue AV Campaigns

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    Rogue antivirus software has recently received extensive attention, justified by the diffusion and efficacy of its propagation. We present a longitudinal analysis of the rogue antivirus threat ecosystem, focusing on the structure and dynamics of this threat and its economics. To that end, we compiled and mined a large dataset of characteristics of rogue antivirus domains and of the servers that host them. The contributions of this paper are threefold. Firstly, we offer the first, to our knowledge, broad analysis of the infrastructure underpinning the distribution of rogue security software by tracking 6,500 malicious domains. Secondly, we show how to apply attack attribution methodologies to correlate campaigns likely to be associated to the same individuals or groups. By using these techniques, we identify 127 rogue security software campaigns comprising 4,549 domains. Finally, we contextualize our findings by comparing them to a different threat ecosystem, that of browser exploits. We underline the profound difference in the structure of the two threats, and we investigate the root causes of this difference by analyzing the economic balance of the rogue antivirus ecosystem. We track 372,096 victims over a period of 2 months and we take advantage of this information to retrieve monetization insights. While applied to a specific threat type, the methodology and the lessons learned from this work are of general applicability to develop a better understanding of the threat economies

    Close Pairs as Proxies for Galaxy Cluster Mergers

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    Galaxy cluster merger statistics are an important component in understanding the formation of large-scale structure. Unfortunately, it is difficult to study merger properties and evolution directly because the identification of cluster mergers in observations is problematic. We use large N-body simulations to study the statistical properties of massive halo mergers, specifically investigating the utility of close halo pairs as proxies for mergers. We examine the relationship between pairs and mergers for a wide range of merger timescales, halo masses, and redshifts (0<z<1). We also quantify the utility of pairs in measuring merger bias. While pairs at very small separations will reliably merge, these constitute a small fraction of the total merger population. Thus, pairs do not provide a reliable direct proxy to the total merger population. We do find an intriguing universality in the relation between close pairs and mergers, which in principle could allow for an estimate of the statistical merger rate from the pair fraction within a scaled separation, but including the effects of redshift space distortions strongly degrades this relation. We find similar behavior for galaxy-mass halos, making our results applicable to field galaxy mergers at high redshift. We investigate how the halo merger rate can be statistically described by the halo mass function via the merger kernel (coagulation), finding an interesting environmental dependence of merging: halos within the mass resolution of our simulations merge less efficiently in overdense environments. Specifically, halo pairs with separations less than a few Mpc/h are more likely to merge in underdense environments; at larger separations, pairs are more likely to merge in overdense environments.Comment: 12 pages, 9 figures; Accepted for publication in ApJ. Significant additions to text and two figures changed. Added new findings on the universality of pair mergers and added analysis of the effect of FoF linking length on halo merger

    Volterra Distortions, Spinning Strings, and Cosmic Defects

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    Cosmic strings, as topological spacetime defects, show striking resemblance to defects in solid continua: distortions, which can be classified into disclinations and dislocations, are line-like defects characterized by a delta function-valued curvature and torsion distribution giving rise to rotational and translational holonomy. We exploit this analogy and investigate how distortions can be adapted in a systematic manner from solid state systems to Einstein-Cartan gravity. As distortions are efficiently described within the framework of a SO(3) {\rlap{\supset}\times}} T(3) gauge theory of solid continua with line defects, we are led in a straightforward way to a Poincar\'e gauge approach to gravity which is a natural framework for introducing the notion of distorted spacetimes. Constructing all ten possible distorted spacetimes, we recover, inter alia, the well-known exterior spacetime of a spin-polarized cosmic string as a special case of such a geometry. In a second step, we search for matter distributions which, in Einstein-Cartan gravity, act as sources of distorted spacetimes. The resulting solutions, appropriately matched to the distorted vacua, are cylindrically symmetric and are interpreted as spin-polarized cosmic strings and cosmic dislocations.Comment: 24 pages, LaTeX, 9 eps figures; remarks on energy conditions added, discussion extended, version to be published in Class. Quantum Gra
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