Titlebook: Nuclear Dynamics: From Quarks to Nuclei; Proceedings of the X M. Teresa Peña,Alfred Stadler,Jiří Adam Conference proceedings 2003 Springer-

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Relativistic Theory of Few-Body Systems, This talk provides an opportunity to review the progress in this field since then. Different methods for the relativistic calculation of few-nucleon systems are briefly described. As an example, seven relativistic calculations of the deuteron elastic structure functions,A.and.,are compared. The cov

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Longitudinal Response Functions for Quasielastic Electron Scattering in Relativistic Nonlinear Modeount RPA correlations. For these calculations, a covariant, consistent, calculation of the nuclear matter linear response has been performed. The effect of the non-linear terms on the longitudinal response has been discussed.

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https://doi.org/10.1007/978-3-7091-6014-5Baryon; Isospin; Meson; Quantum mechanics; Quark; collision; hadron; scattering; spectra; topological soliton

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978-3-7091-7301-5Springer-Verlag Wien 2003

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,The Importance of the Final-State Interaction in , →, near Threshold,tion is highly dependent on the reaction mechanism, its shape is essentially determined by the ηd final-state interaction. This strong signature provides information about the ηN scattering length. We found that the np —ηd experimental data can only be explained if the ηN scattering length has a small real part.

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Search For the Quark Shell Structure Using the Non-Topological Soliton Model,on solutions are obtained self-consistently. We show that the baryon number density lias point-like symmetries and the corresponding valence quark spectrum of the lowest energy exhibits approximate four-fold degenerate. Our results indicate the possibility of existence of the shell-like structure in the multi-baryonic system.

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Baryons as Relativistic Three-Quark Systems,e address the issues of excitation spectra, electroweak structure, and mesonic resonance decays. The necessities of implementing simultaneously the symmetries of low-energy quantum chromodynamics and of relativistic invariance are emphasized.

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