6,641 research outputs found

    Multipole moments in Kaluza-Klein theories

    Get PDF
    This paper contains discussion of the problem of motion of extended i.e. non point test bodies in multidimensional space. Extended bodies are described in terms of so called multipole moments. Using approximated form of equations of motion for extended bodies deviation from geodesic motion is derived. Results are applied to special form of space-time.Comment: 11 pages, AMS-TeX, few misprints corrected, to appear in Classical and Quantum Gravit

    Semileptonic charm decays D \to \pi l \nu_{\l} and D→KlνlD \to K l \nu_l from QCD Light-Cone Sum Rules

    Full text link
    We present a new calculation of the D→πD\to\pi and D→KD \to K form factors from QCD light-cone sum rules. The MS‾\overline{MS} scheme for the cc-quark mass is used and the input parameters are updated. The results are fDπ+(0)=0.67−0.07+0.10f^+_{D\pi}(0)= 0.67^{+0.10}_{-0.07}, fDK+(0)=0.75−0.08+0.11f^+_{DK}(0)=0.75^{+0.11}_{-0.08} and fDπ+(0)/fDK+(0)=0.88±0.05f^+_{D\pi}(0)/f^+_{DK}(0)=0.88 \pm 0.05. Combining the calculated form factors with the latest CLEO data, we obtain ∣Vcd∣=0.225±0.005±0.003−0.012+0.016|V_{cd}|=0.225\pm 0.005 \pm 0.003 ^{+0.016}_{-0.012} and ∣Vcd∣/∣Vcs∣=0.236±0.006±0.003±0.013|V_{cd}|/|V_{cs}|= 0.236\pm 0.006\pm 0.003\pm 0.013 where the first and second errors are of experimental origin and the third error is due to the estimated uncertainties of our calculation. We also evaluate the form factors fDπ−f^-_{D\pi} and fDK−f^-_{DK} and predict the slope parameters at q2=0q^2=0. Furthermore, calculating the form factors from the sum rules at q2<0q^2<0, we fit them to various parameterizations. After analytic continuation, the shape of the D→π,KD\to \pi,K form factors in the whole semileptonic region is reproduced, in a good agreement with experiment.Comment: 34 pages, 5 figure

    Form Factors and Strong Couplings of Heavy Baryons from QCD Light-Cone Sum Rules

    Full text link
    We derive QCD light-cone sum rules for the hadronic matrix elements of the heavy baryon transitions to nucleon. In the correlation functions the Λc,Σc\Lambda_c,\Sigma_c and Λb\Lambda_b -baryons are interpolated by three-quark currents and the nucleon distribution amplitudes are used. To eliminate the contributions of negative parity heavy baryons, we combine the sum rules obtained from different kinematical structures. The results are then less sensitive to the choice of the interpolating current. We predict the Λb→p\Lambda_{b}\to p form factor and calculate the widths of the Λb→pℓνl\Lambda_{b}\to p\ell\nu_l and Λb→pπ\Lambda_{b}\to p \pi decays. Furthermore, we consider double dispersion relations for the same correlation functions and derive the light-cone sum rules for the ΛcND(∗)\Lambda_cND^{(*)} and ΣcND(∗)\Sigma_cND^{(*)} strong couplings. Their predicted values can be used in the models of charm production in ppˉp\bar{p} collisions.Comment: 45 pages, 3 figure

    Geodesic Deviation in Kaluza-Klein Theories

    Full text link
    We study in detail the equations of the geodesic deviation in multidimensional theories of Kaluza-Klein type. We show that their 4-dimensional space-time projections are identical with the equations obtained by direct variation of the usual geodesic equation in the presence of the Lorentz force, provided that the fifth component of the deviation vector satisfies an extra constraint derived here.Comment: 5 pages, Revtex, 1 figure. To appear in Phys. Rev. D (Brief Report

    A multi-wavelength study of a double intermediate-mass protostar - from large-scale structure to collimated jets

    Full text link
    (abridged) We study a previously discovered protostellar source that is deeply embedded and drives an energetic molecular outflow. The source, UYSO1, is located close to IRAS 07029-1215 at a distance of ~1 kpc. The multi-wavelength observations resulted in the detection of a double intermediate-mass protostar at the location of UYSO1. In addition to the associated molecular outflow, with a projected size of 0.25 pc, two intersecting near-infrared jets with projected sizes of 0.4 pc and 0.2 pc were found. However, no infrared counterparts to the driving sources could be detected in sensitive near- to far-infrared observations. In interferometric millimeter observations, UYSO1 was resolved into two continuum sources with high column densities and gas masses of 3.5 Mo and 1.2 Mo, with a linear separation of 4200 AU. We report the discovery of a H2O maser toward one of the two sources. The total luminosity is roughly estimated to be ~50 Lo, shared by the two components, one of which is driving the molecular outflow that has a dynamical timescale of less than a few thousand years. The jets of the two individual components are not aligned. Submillimeter observations show that the region lacks typical hot-core chemistry. We thus find two protostellar objects, whose associated circumstellar and parent core masses are high enough to suggest that they may evolve into intermediate-mass stars. This is corroborated by their association with a very massive and energetic CO outflow, suggesting high protostellar accretion rates. The short dynamical timescale of the outflow, the pristine chemical composition of the cloud core and absence of hot core tracers, the absence of detectable radio continuum emission, and the very low protostellar luminosity argue for an extremely early evolutionary stage.Comment: 10 pages, 10 figures, accepted for publication in A&A; minor changes: typos corrected, revised argument in Section

    First Detection of Millimeter Dust Emission from Brown Dwarf Disks

    Full text link
    We report results from the first deep millimeter continuum survey targeting Brown Dwarfs (BDs). The survey led to the first detection of cold dust in the disks around two young BDs (CFHT-BD-Tau 4 and IC348 613), with deep JCMT and IRAM observations reaching flux levels of a few mJy. The dust masses are estimated to be a few Earth masses assuming the same dust opacities as usually applied to TTauri stars.Comment: 5 pages, accepted for ApJ

    The Collapse of Large Extra Dimensions

    Get PDF
    In models of spacetime that are the product of a four-dimensional spacetime with an ``extra'' dimension, there is the possibility that the extra dimension will collapse to zero size, forming a singularity. We ask whether this collapse is likely to destroy the spacetime. We argue, by an appeal to the four-dimensional cosmic censorship conjecture, that--at least in the case when the extra dimension is homogeneous--such a collapse will lead to a singularity hidden within a black string. We also construct explicit initial data for a spacetime in which such a collapse is guaranteed to occur and show how the formation of a naked singularity is likely avoided.Comment: Uses revtex

    The electronic structure of amorphous silica: A numerical study

    Full text link
    We present a computational study of the electronic properties of amorphous SiO2. The ionic configurations used are the ones generated by an earlier molecular dynamics simulations in which the system was cooled with different cooling rates from the liquid state to a glass, thus giving access to glass-like configurations with different degrees of disorder [Phys. Rev. B 54, 15808 (1996)]. The electronic structure is described by a tight-binding Hamiltonian. We study the influence of the degree of disorder on the density of states, the localization properties, the optical absorption, the nature of defects within the mobility gap, and on the fluctuations of the Madelung potential, where the disorder manifests itself most prominently. The experimentally observed mismatch between a photoconductivity threshold of 9 eV and the onset of the optical absorption around 7 eV is interpreted by the picture of eigenstates localized by potential energy fluctuations in a mobility gap of approximately 9 eV and a density of states that exhibits valence and conduction band tails which are, even in the absence of defects, deeply located within the former band gap.Comment: 21 pages of Latex, 5 eps figure

    The R.I. Pimenov unified gravitation and electromagnetism field theory as semi-Riemannian geometry

    Full text link
    More then forty years ago R.I. Pimenov introduced a new geometry -- semi-Riemannian one -- as a set of geometrical objects consistent with a fibering pr:Mn→Mm. pr: M_n \to M_m. He suggested the heuristic principle according to which the physically different quantities (meter, second, coulomb etc.) are geometrically modelled as space coordinates that are not superposed by automorphisms. As there is only one type of coordinates in Riemannian geometry and only three types of coordinates in pseudo-Riemannian one, a multiple fibered semi-Riemannian geometry is the most appropriate one for the treatment of more then three different physical quantities as unified geometrical field theory. Semi-Euclidean geometry 3R54^{3}R_5^4 with 1-dimensional fiber x5x^5 and 4-dimensional Minkowski space-time as a base is naturally interpreted as classical electrodynamics. Semi-Riemannian geometry 3V54^{3}V_5^4 with the general relativity pseudo-Riemannian space-time 3V4,^{3}V^4, and 1-dimensional fiber x5,x^5, responsible for the electromagnetism, provides the unified field theory of gravitation and electromagnetism. Unlike Kaluza-Klein theories, where the 5-th coordinate appears in nondegenerate Riemannian or pseudo-Riemannian geometry, the theory based on semi-Riemannian geometry is free from defects of the former. In particular, scalar field does not arise. PACS: 04.50.Cd, 02.40.-k, 11.10.KkComment: 16 pages, 2 figures. Submited to Physics of Atomic Nucle
    • …
    corecore