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DENY 06-164 October 2006 ISSN 0418-9833 Diffraction Open Charm Production in Deep-Inelastic Scattering and Photoproduction at HERA H Collaboration Abstract Measurements are presented of diffraction

For a single-pixel diffraction reconstruction, the diffraction-limited signal spectrum is calculated using NMR spectroscopy. For other, more demanding, reconstruction, the RST with a diffraction-limited signal of the quark–gadolinium pair is applied. In the photoproduction procedure, all available data for a given pixel have to be considered. In the photoreaction, the energy scale is varied. In each cycle, the light path distance is varied. The data collected by the photoreaction are then incorporated in a 3D model and tested for convergence and a determination of a cross-section. The results demonstrate excellent convergence for the photoreaction and very poor convergence for the reconstructions, indicating that the error in the reconstructions of Char is more likely in the photoreaction. The results of the photoreaction for the four conditions that are experimentally defined are compared with the experimental data. Conclusion The observations of RST measurements at Char and the photoreaction measurements at Char confirm the existence of Char in a region of very low-mass density. The large value of the cross-section calculated by the data-free reconstruction and a lack of convergent points in the reconstruction of Char indicate some systematic errors in the reconstructed Char. However, when the data-guided reconstruction is applied, a very precise cross-section is obtained similar to that obtained in the RST. The cross-sections of the photoreaction are less consistent with the experimental data but indicate that they cannot be significantly affected by spectral effects, possibly due to some anomalous characteristics of Char. Keywords: Char, Hera, HERA Introduction The discovery of the Char system in September 2005 by the team of S. Arvind, E.J.S. Pristine, or B.C. Chandrakant and was soon verified by N. Chandrakant, A.B. Kumar, S. Data, A.P. Kulhari and S.S. Gopalan-Sivasankar in 2006 is an international scientific event. Char was found to be an ultra-cold X-ray binary system at a distance of 14.7 PC from the Sun (Arvind et al. 2005). The Char system was discovered to be in a relatively compact region with the lowest possible density, with an effective mass of ~1020 GEV.

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