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    Search for NN-decoupled dibaryons using the process ppγγXpp \to \gamma \gamma X below the pion production threshold

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    The energy spectrum for high energy γ\gamma-rays (Eγ10E_\gamma \geq 10 MeV) from the process ppγγXpp \to \gamma \gamma X emitted at 90090^0 in the laboratory frame has been measured at an energy below the pion production threshold, namely, at 216 MeV. The resulting photon energy spectrum extracted from γγ\gamma-\gamma coincidence events consists of a narrow peak at a photon energy of about 24 MeV and a relatively broad peak in the energy range of (50 - 70) MeV. The statistical significances for the narrow and broad peaks are 5.3σ\sigma and 3.5σ\sigma, respectively. This behavior of the photon energy spectrum is interpreted as a signature of the exotic dibaryon resonance d1d^\star_1 with a mass of about 1956 MeV which is assumed to be formed in the radiative process ppγd1pp \to \gamma d^\star_1 followed by its electromagnetic decay via the d1ppγd^\star_1 \to pp \gamma mode. The experimental spectrum is compared with those obtained by means of Monte Carlo simulations.Comment: 14 pages, LaTex, 6 eps-figures, accepted for publication in Phys.Rev.
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