Abstract

Results of a partial wave analysis of new high-statistics data on γp→pηγp\to pη from MAMI are presented. A fit using known broad resonances and only standard background amplitudes can not describe the relatively narrow peaking structure in the cross section in the mass region of 1660-1750 MeV which follows a minimum. An improved description of the data can be reached by either assuming the existence of a narrow resonance at a mass of about 1700 MeV with small photo-coupling or by a threshold effect. In the latter case the observed structure is explained by a strong (resonant or non-resonant) γp→ωpγp\toωp coupling in the S11S_{11} partial wave. When the beam asymmetry data, published by part of the GRAAL collaboration, are included in the fit, the solution with a narrow P11P_{11} state is slightly preferred. In that fit, mass and width of the hypothetical resonance are determined to M∼M\sim1694 MeV and Γ∼40Γ\sim 40 MeV, respectively, and the photo-coupling to BrηNA1/2p∼2.6⋅10−3\sqrt{{\rm Br}_{ηN}} A_{1/2}^p \sim 2.6\cdot 10^{-3} GeV−1/2^{-1/2}. High precision measurements of the target asymmetry and FF-observable are mandatory to establish the possible existence of such a narrow state and to provide the necessary information to define which partial wave is responsible for the structure observed in the data.

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