1,129 research outputs found

    Multipole Extraction: A novel, model independent method

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    A novel method for extracting multipole amplitudes in the nucleon resonance region from electroproduction data is presented. The method is based on statistical concepts and it relies heavily on Monte Carlo and simulation techniques; it produces precise identification and determination of the contributing multipole amplitudes in the resonance region and for the first time a rigorous determination of the associated experimental uncertainty. The results are demonstrated to be independent of any model bias. The method is applied in the reanalysis of the Q2=0.127GeV2/c2Q^{2}=0.127 GeV^2/c^2 Bates and Mainz N→ΔN\to \Delta data.Comment: Proceedings, "Shape of Hadrons" Workshop, 27-29 April 2006, Athens, GREEC

    On hadron deformation: a model independent extraction of EMR from pion photoproduction data

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    The multipole content of pion photoproduction at the Δ+(1232)\Delta^+ (1232) resonance has been extracted from a data set dominated by recent Mainz Microtron (MAMI) precision measurements. The analysis has been carried out in the Athens Model Independent Analysis Scheme (AMIAS), thus eliminating any model bias. The benchmark quantity for nucleon deformation, EMR=E2/M1=E1+3/2/M1+3/2EMR = E2/M1 = E_{1+}^{3/2}/M_{1+}^{3/2}, was determined to be −2.5±0.4stat+syst-2.5 \pm 0.4_{stat+syst}, thus reconfirming in a model independent way that the conjecture of baryon deformation is valid. The derived multipole amplitudes provide stringent constraints on QCD simulations and QCD inspired models striving to describe hadronic structure. They are in good agreement with phenomenological models which explicitly incorporate pionic degrees of freedom and with lattice QCD calculations.Comment: 14 pages, 9 figures, 2 table

    Energy Dependence of the Delta Resonance: Chiral Dynamics in Action

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    There is an important connection between the low energy theorems of QCD and the energy dependence of the Delta resonance in pi-N scattering, as well as the closely related gamma^{*} N -> pi N reaction. The resonance shape is due not only to the strong pi-N interaction in the p wave but the small interaction in the s wave; the latter is due to spontaneous chiral symmetry breaking in QCD (i.e. the Nambu-Goldstone nature of the pion). A brief overview of experimental tests of chiral perturbation theory and chiral based models is presentedComment: 11 pages, 6 figures, Festschrift for S.N. yan

    Measurements of the Generalized Electric and Magnetic Polarizabilities of the Proton at Low Q2 Using the VCS Reaction

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    The mean square polarizability radii of the proton have been measured for the first time in a virtual Compton scattering experiment performed at the MIT-Bates out-of-plane scattering facility. Response functions and polarizabilities obtained from a dispersion analysis of the data at Q2=0.06 GeV2/c2 are in agreement with O(p3) heavy baryon chiral perturbation theory. The data support the dominance of mesonic effects in the polarizabilities, and the increase of beta with increasing Q2 is evidence for the cancellation of long-range diamagnetism by short-range paramagnetism from the pion cloud

    Refractive elastic scattering of carbon and oxygen nuclei: The mean field analysis and Airy structures

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    The experimental data on the 16^{16}O+12+^{12}C and 18^{18}O+12+^{12}C elastic scatterings and their optical model analysis are presented. Detailed and complete elastic angular distributions have been measured at the Strasbourg Vivitron accelerator at several energies covering the energy range between 5 and 10 MeV per nucleon. The elastic scattering angular distributions show the usual diffraction pattern and also, at larger angles, refractive effects in the form of nuclear rainbow and associated Airy structures. The optical model analysis unambiguously shows the evolution of the refractive scattering pattern. The observed structure, namely the Airy minima, can be consistently described by a nucleus-nucleus potential with a deep real part and a weakly absorptive imaginary part. The difference in absorption in the two systems is explained by an increased imaginary (mostly surface) part of the potential in the 18^{18}O+12+^{12}C system. The relation between the obtained potentials and those reported for the symmetrical 16^{16}O+16+^{16}O and 12^{12}C+12+^{12}C systems is drawn.Comment: 10 pages, 9 figures, Phys. rev. C in pres
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