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| Microscopic Models of Heavy Ion Interactions 1 Introducuon 2 High-Energy Scattering: Ha(ironic Picture 3 Microscopic String Models 4 Nuclear Stopping 5 Hyperon and Antihyperon Production 6 J/ч Suppression 7 Conclusions Appendix A Ultrarelativistic Nucleus-Nucleus Collisions and the Quark-Gluon Plasma A. Andronic, P. Braun-Munzinger 1 Introduction 2 Theoretical Background 3 Experimental Program and Global Observables 4 Particle Yields and Their Statistical Description 5 Charmonium and Charmed Hadrons 6 Outlook Nuclear Physics Far from Stability K. Heyde 1 Introduction: Physics of Nuclear Binding and Stability 2 Exploring the Nuclear Many-Body System: Learning from the Past 3 Theoretical Approaches for Describing Atomic Nuclei near Stability 4 How Far Can One Extrapolate the Nuclear Shell-Model? 5 Exploring the Nuclear Many-Body System: Recent Experimental Results 6 Outlook Experiments with Radioactive Nuclear Beams 1 Introduction 2 Production and Acceleration of Exotic Nuclei 3 Experimental Studies of Halo States 4 Nuclei at and Beyond the Driplines 5 Beta-Decay of Exotic Nuclei 6 Suggestions for Further Reading Beyond the Proton Drip-Line 1 Introduction 2 The Proton Drip-Line 3 Proton Radioactivity from Spherical Nuclei 4 Proton Radioactivity from Deformed Nuclei 5 Conclusions Nuclear Reactions with Exotic Beams 1 Introduction 2 Heavy-Ion Reactions and Optical Potentialsin Systems Far from the Stability Line. Effects Associated with the Presence of Skins and Haloes 3 Consequences of a Neutron Skin on the Properties of the Nuclear Excitation States. Giant Resonances and Novel Collective Modes 4 Low-Lying Strength (Mainly Dipole) for Weakly Bound Systen at the Drip Lines. Effect of Halo Distribution and Break-Up Processes 5 Sub-barrier Fusion Processes with Weakly-Bound Nuclei. Effect of Coupling to the Continuum Nuclear Astrophysics: Selected Topics 1 Introduction 2 The Nuclear Physics Input 3 Hydrostatic Burning Stages 4 Core Collapse Supernovae 5 Nucleosynthesis Beyond Iron Equation of State of Hypernuclear Matter and Neutron Ste 1 introduction 2 The Baryon-Baryon Interaction and the Nuclear Many-Body Problem 3 /3-Stability in Neutron Star Matter …… Regularity and Chaos in the Nuclear Masses An Introduction to Nuclear Supersymmetry:A Unification Scheme for Nuclei Index |
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