447 research outputs found

    Evidence for narrow resonant structures at W1.68W \approx 1.68 and W1.72W \approx 1.72 GeV in real Compton scattering off the proton

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    First measurement of the beam asymmetry Σ\Sigma for Compton scattering off the proton in the energy range Eγ=0.851.25E_{\gamma}=0.85 - 1.25 GeV is presented. The data reveals two narrow structures at Eγ=1.036E_{\gamma}= 1.036 and Eγ=1.119E_{\gamma}=1.119 GeV. They may signal narrow resonances with masses near 1.681.68 and 1.721.72 GeV, or they may be generated by the sub-threshold KΛK\Lambda and ωp\omega p production. Their decisive identification requires additional theoretical and experimental efforts.Comment: Published versio

    Eta photoproduction off the neutron at GRAAL: Evidence for a resonant structure at W=1.67 GeV

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    New (preliminary) data on eta photoproduction off the neutron are presented. These data reveal a resonant structure at W=1.67 GeV.Comment: 8 pages, 4 figures. Published in Proceedings of Workshop on the Physics of Excited Nucleons NSTAR2004, Grenoble, France, March 24 - 27, pg.19

    Eta photoproduction off the neutron at GRAAL

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    The gamma n -> eta n quasi-free cross section reveals a resonant structure at W ~ 1.675 GeV. This structure may be a manifestation of a baryon resonance. A priori its properties, the possibly narrow width and the strong photocoupling to the neutron, look surprising. This structure may also signal the existence of a narrow state.Comment: To appear in Proceedings of Workshop on the Physics of Excited Nucleons NSTAR2005, 12 - 15 October 2005, Tallahassee, Florida, US

    Evidence for Narrow N*(1685) Resonance in Quasifree Compton Scattering on the Neutron

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    The first study of quasi-free Compton scattering on the neutron in the energy range of Eγ=0.751.5E_{\gamma}=0.75 - 1.5 GeV is presented. The data reveals a narrow peak at W1.685W\sim 1.685 GeV. This result, being considered in conjunction with the recent evidence for a narrow structure at W1.68W\sim 1.68GeV in the η\eta photoproduction on the neutron, suggests the existence of a new nucleon resonance with unusual properties: the mass M1.685M\sim 1.685GeV, the narrow width Γ30\Gamma \leq 30MeV, and the much stronger photoexcitation on the neutron than on the proton.Comment: Replaced with the version published in Phys. Rev.

    Eta photoproduction on the neutron at GRAAL: Measurement of the differential cross section

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    In this contribution, we will present our first preliminary measurement of the differential cross section for the reaction gamma+n->eta+n. Comparison of the reactions gamma+p->eta+p for free and bound proton (D2 target) will also be discussed.Comment: 6 pages, 4 figures, Proceedings of the 10th International Symposium on Meson-Nucleon Physics and the Structure of the Nucleon, August 29-September 4 2004, Beijing, Chin

    Limits on light-speed anisotropies from Compton scattering of high-energy electrons

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    The possibility of anisotropies in the speed of light relative to the limiting speed of electrons is considered. The absence of sidereal variations in the energy of Compton-edge photons at the ESRF's GRAAL facility constrains such anisotropies representing the first non-threshold collision-kinematics study of Lorentz violation. When interpreted within the minimal Standard-Model Extension, this result yields the two-sided limit of 1.6 x 10^{-14} at 95% confidence level on a combination of the parity-violating photon and electron coefficients kappa_{o+} and c. This new constraint provides an improvement over previous bounds by one order of magnitude.Comment: 4 pages, 4 figure

    Lowering the Light Speed Isotropy Limit: European Synchrotron Radiation Facility Measurements

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    The measurement of the Compton edge of the scattered electrons in GRAAL facility in European Synchrotron Radiation Facility (ESRF) in Grenoble with respect to the Cosmic Microwave Background dipole reveals up to 10 sigma variations larger than the statistical errors. We now show that the variations are not due to the frequency variations of the accelerator. The nature of Compton edge variations remains unclear, thus outlining the imperative of dedicated studies of light speed anisotropy
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