Peter Egelhof GSI Darmstadt, Germany 8th. International ... - Bulgaria

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Introduction: Phenomena and Burning Questions
Introduction: Phenomena and Burning QuestionsThe challenge: For the understanding of nucleosynthesis and stellar dynamics weneed to know properties of many exotic nuclei.Nuclear input: half lives, masses, reaction ratesAstrophysical calculationsComparison to observationrapid proton capture(rapid neutron capture )
Page 1 and 2: Nuclear Structure Studies on Exotic
Page 3 and 4: I. Introductionmethods of nuclear s
Page 5 and 6: Introduction: Phenomena and Burning
Page 9 and 10: Halo-Nuclei - a New Phenomenonof th
Page 11 and 12: The Radial Shape of Nuclei: from St
Page 15 and 16: The Collective Response of the Nucl
Page 17 and 18: The Collective Response of the Nucl
Page 19 and 20: The Radial Shape of Nuclei: from St
Page 21 and 22: New Magic Number N = 16N=20 shell g
Page 23: Introduction: Phenomena and Burning
Page 27 and 28: Light-Ion Induced Direct Reactions
Page 29 and 30: The Present Radioactive Beam Facili
Page 31 and 32: Production of Radioactive Beams at
Page 33 and 34: Why Fast Radioactive Beams?Producti
Page 35 and 36: II. Experimental TechniquesExperime
Page 37 and 38: Application of Active TargetsConcep
Page 39 and 40: The Experimental Storage Ring ESR a

Peter Egelhof GSI Darmstadt, Germany 8th. International ... - Bulgaria

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