5,741 research outputs found

    VMD, the WZW Lagrangian and ChPT: The Third Mixing Angle

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    We show that the Hidden Local Symmetry Model, supplemented with well-known procedures for breaking flavor SU(3) and nonet symmetry, provides all the information contained in the standard Chiral Perturbation Theory (ChPT) Lagrangian L(0)+L(1){\cal L}^{(0)}+{\cal L}^{(1)}. This allows to rely on radiative decays of light mesons (VPγVP\gamma and PγγP \gamma\gamma) in order to extract some numerical information of relevance to ChPT: a value for Λ1=0.20±0.04\Lambda_1=0.20 \pm 0.04, a quark mass ratio of 21.2±2.4\simeq 21.2 \pm 2.4, and a negligible departure from the Gell-Mann--Okubo mass formula. The mixing angles are θ8=20.40±0.96\theta_8=-20.40^\circ \pm 0.96^\circ and θ0=0.05±0.99\theta_0=-0.05^\circ \pm 0.99^\circ. We also give the values of all decay constants. It is shown that the common mixing pattern with one mixing angle θP\theta_P is actually quite appropriate and algebraically related to the η/η\eta/\eta' mixing pattern presently preferred by the ChPT community. For instance the traditional θP\theta_P is functionally related to the ChPT θ8\theta_8 and fulfills θPθ8/2\theta_P \simeq \theta_8/2. The vanishing of θ0\theta_0, supported by all data on radiative decays, gives a novel relation between mixing angles and the violation of nonet symmetry in the pseudoscalar sector. Finally, it is shown that the interplay of nonet symmetry breaking through U(3) \ra SU(3)×\times U(1) satisfies all requirements of the physics of radiative decays without any need for additional glueballs.Comment: 31 pages, 1 figur

    Isospin Symmetry Breaking within the HLS Model: A Full (ρ,ω,ϕ\rho, \omega, \phi) Mixing Scheme

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    We study the way isospin symmetry violation can be generated within the Hidden Local Symmetry (HLS) Model. We show that isospin symmetry breaking effects on pseudoscalar mesons naturally induces correspondingly effects within the physics of vector mesons, through kaon loops. In this way, one recovers all features traditionally expected from \rho-\omg mixing and one finds support for the Orsay phase modelling of the e^+e^- \ra \pi^+ \pi^- amplitude. We then examine an effective procedure which generates mixing in the whole ρ\rho, \omg, ϕ\phi sector of the HLS Model. The corresponding model allows us to account for all two body decays of light mesons accessible to the HLS model in modulus and phase, leaving aside the \rho \ra \pi \pi and K^* \ra K \pi modes only, which raise a specific problem. Comparison with experimental data is performed and covers modulus and phase information; this represents 26 physics quantities successfully described with very good fit quality within a constrained model which accounts for SU(3) breaking, nonet symmetry breaking in the pseudoscalar sector and, now, isospin symmetry breaking.Comment: 38 pages, version published in Eur. Phys. J.

    Direct CP Violation in B±ρ±π+πB^\pm\to\rho^\pm\pi^+\pi^- in the ρ0\rho^0-ω\omega Interference Region

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    We study direct CP violation in B±ρ±ρ0(ω)ρ±π+πB^\pm \to \rho^\pm\rho^0(\omega) \to \rho^\pm\pi^+\pi^- and focus specifically on the rate asymmetry in the ρ0\rho^0-ω\omega interference region. Here the strong phase is dominated by isospin violation, so that it can be essentially determined by e+eρ0(ω)π+πe^+e^- \to \rho^0 (\omega) \to \pi^+\pi^- data. We find the CP-violating asymmetry to be of the order of 20% at the ω\omega invariant mass. Moreover, it is robust with respect to the estimable strong-phase uncertainties, permitting the extraction of sinα\sin\alpha from this channel.Comment: 4 pages, LaTeX, aipproc.sty, talk presented at CIPANP97, Big Sky, M

    Analysis of permanent magnets as elasmobranch bycatch reduction devices in hook-and-line and longline trials

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    Previous studies indicate that elasmobranch fishes (sharks, skates and rays) detect the Earth’s geomagnetic field by indirect magnetoreception through electromagnetic induction, using their ampullae of Lorenzini. Applying this concept, we evaluated the capture of elasmobranchs in the presence of permanent magnets in hook-and-line and inshore longline fishing experiments. Hooks with neodymium-iron-boron magnets significantly reduced the capture of elasmobranchs overall in comparison with control and procedural control hooks in the hook-and-line experiment. Catches of Atlantic sharpnose shark (Rhizoprionodon terraenovae) and smooth dogfish (Mustelus canis) were signif icantly reduced with magnetic hook-and-line treatments, whereas catches of spiny dogfish (Squalus acanthias) and clearnose skate (Raja eglanteria) were not. Longline hooks with barium-ferrite magnets significantly reduced total elasmobranch capture when compared with control hooks. In the longline study, capture of blacktip sharks (Carcharhinus limbatus) and southern stingrays (Dasyatis americana) was reduced on magnetic hooks, whereas capture of sandbar shark (Carcharhinus plumbeus) was not affected. Teleosts, such as red drum (Sciaenops ocellatus), Atlantic croaker (Micropogonias undulatus), oyster toadfish (Opsanus tau), black sea bass (Centropristis striata), and the bluefish (Pomatomas saltatrix), showed no hook preference in either hook-and-line or longline studies. These results indicate that permanent magnets, although eliciting species-specific capture trends, warrant further investigation in commercial longline and recreational fisheries, where bycatch mortality is a leading contributor to declines in elasmobranch populations

    Constraints on New Physics from Baryogenesis and Large Hadron Collider Data

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    We demonstrate the power of constraining theories of new physics by insisting that they lead to electroweak baryogenesis, while agreeing with current data from the Large Hadron Collider. The general approach is illustrated with a singlet scalar extension of the Standard Model. Stringent bounds can already be obtained, which reduce the viable parameter space to a small island.Comment: 4 pages, 2 figures. References added, figures updated. Version to appear in PR

    A Note on Frame Dragging

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    The measurement of spin effects in general relativity has recently taken centre stage with the successfully launched Gravity Probe B experiment coming toward an end, coupled with recently reported measurements using laser ranging. Many accounts of these experiments have been in terms of frame-dragging. We point out that this terminology has given rise to much confusion and that a better description is in terms of spin-orbit and spin-spin effects. In particular, we point out that the de Sitter precession (which has been mesured to a high accuracy) is also a frame-dragging effect and provides an accurate benchmark measurement of spin-orbit effects which GPB needs to emulate

    RascalC: A Jackknife Approach to Estimating Single and Multi-Tracer Galaxy Covariance Matrices

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    To make use of clustering statistics from large cosmological surveys, accurate and precise covariance matrices are needed. We present a new code to estimate large scale galaxy two-point correlation function (2PCF) covariances in arbitrary survey geometries that, due to new sampling techniques, runs 104\sim 10^4 times faster than previous codes, computing finely-binned covariance matrices with negligible noise in less than 100 CPU-hours. As in previous works, non-Gaussianity is approximated via a small rescaling of shot-noise in the theoretical model, calibrated by comparing jackknife survey covariances to an associated jackknife model. The flexible code, RascalC, has been publicly released, and automatically takes care of all necessary pre- and post-processing, requiring only a single input dataset (without a prior 2PCF model). Deviations between large scale model covariances from a mock survey and those from a large suite of mocks are found to be be indistinguishable from noise. In addition, the choice of input mock are shown to be irrelevant for desired noise levels below 105\sim 10^5 mocks. Coupled with its generalization to multi-tracer data-sets, this shows the algorithm to be an excellent tool for analysis, reducing the need for large numbers of mock simulations to be computed.Comment: 29 pages, 8 figures. Accepted by MNRAS. Code is available at http://github.com/oliverphilcox/RascalC with documentation at http://rascalc.readthedocs.io
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