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4.3 Nuclear Structure and Dynamics since spring 2010, thus completing more than 10 years of R&D on gamma-ray tracking. The joint European AGATA collaboration is currently in the process of securing funding for the construction of 1/3 of AGATA by 2013. The completion of this stage and the realisation of the full AGATA spectrometer is recognized to be of utmost importance for the successful exploitation of present and future radioactive and stable-ion beam facilities. Theory initiative New project for advanced studies in theoretical nuclear structure and reaction physics of exotic nuclei bringing together theorists, computer scientists and experimentalists to support and stimulate experimental research performed at the European facilities To meet the challenges brought by the new area of nuclei accessed by future experimental facilities, all theoretical models will have to progress in several directions. Many questions can only be addressed by a strong coordination of the often small theory groups working in Europe and having a strong expertise in specific models. To bring the necessary support to the experimental facilities, a new project unifying all the individual efforts should be launched in Europe in the near future. This project for advanced studies in theoretical nuclear structure and reaction physics of exotic nuclei must bring together theorists, computer scientists and experimentalists to support and stimulate experimental research performed at the European facilities to define new research directions, and to encourage and shepherd international scientific collaborations between low-energy nuclear theory groups in Europe. The principal thrust should come from the existing and future large European infrastructure facilities which should integrate theory to a much higher degree as compared to the present situation. ECT* in Trento must be supported in its leading role as a training centre for young researchers, and an international venue for scientific meetings that involve both theorists and experimentalists from all domains of nuclear physics, and related fields. 128 | Perspectives of Nuclear Physics in Europe – NuPECC Long Range Plan 2010
4. Scientific Themes 4.4 Nuclear Astrophysics Convener: Brian Fulton (York) Nicolas Chamel (Bruxelles), Zsolt Fülöp (Debrecen), Fairouz Hammache (Orsay), Michael Heil (Darmstadt), Jordi José (Barcelona), Gabriel Martinez Pinedo (Darmstadt), Francois de Oliveira (Caen), Paolo Prati (Genova), Thomas Rauscher (Basel), Stefano Romano (Catania), Kerstin Sonnabend (Darmstadt), Christof Vockenhuber (Zürich), Phil Woods (Edinburgh) NuPECC Steering Committee Member: Paul-Henri Heenen NuPECC Liaison: Sotirios Harissopulos
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Forward Look Perspectives of Nuclea
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Contents Foreword 3 1. Executive Su
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Foreword The goal of this European
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1. Executive Summary 1.1.3 Objectiv
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1. Executive Summary structure and
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1. Executive Summary using slow ant
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1. Executive Summary The role of gl
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1. Executive Summary from the few-b
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1. Executive Summary Advances in nu
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1. Executive Summary and AMS or hig
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2. Recommendations and Roadmap EURI
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3. Research Infrastructures and Net
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4. Scientific Themes 4.1 Hadron Phy
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4.1.2 Basic Properties of Quantum C
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coupling can be applied. A key tool
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opportunity to determine the moduli
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A broad experimental programme has
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4.1.4 Hadron Spectroscopy Recent Ac
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Physics Perspectives There is a mul
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Global Perspective and Efforts In t
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The longest-range parts of these fo
Page 79 and 80: concentrate their efforts and conti
Page 81 and 82: 4. Scientific Themes 4.2 Phases of
Page 83 and 84: tion of state would therefore deter
Page 85 and 86: an increase at the deconfinement te
Page 87 and 88: can be described with statistical h
Page 89 and 90: Box 3. Heavy ion fragmentation and
Page 91 and 92: Figure 7. Isotopic dependence of th
Page 93 and 94: energies so far did not find indica
Page 95 and 96: 4.2.5 The High-Energy Frontier The
Page 97 and 98: Figure 10. Elliptic flow parameter
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Page 101 and 102: the same time being able to precise
Page 103 and 104: technology), a three-dimensional ar
Page 105 and 106: 4. Scientific Themes 4.3 Nuclear St
Page 107 and 108: 4.3.2 Theoretical Aspects Ab Initio
Page 109 and 110: the continuum, as done, e.g., in th
Page 111 and 112: Each of these extensions will open
Page 113 and 114: Halos, clusters and few-body correl
Page 115 and 116: Figure 3. Mirror Energy Differences
Page 117 and 118: Superheavy elements The existence o
Page 119 and 120: Figure 5. Gamma-ray spectrum of the
Page 121 and 122: The experimental evidence for the e
Page 123 and 124: 4.3.7 Ground-State Properties Figur
Page 125 and 126: For nuclear astrophysics applicatio
Page 127 and 128: A detector array for high-energy ph
Page 129: and rejection power of separators.
Page 133 and 134: powers many of the objects we obser
Page 135 and 136: Hydrostatic burning Stars spend the
Page 137 and 138: Significant uncertainties remain fo
Page 139 and 140: nova ejecta (a few seconds). In thi
Page 141 and 142: have to be calculated. Current micr
Page 143 and 144: An improvement in the precision of
Page 145 and 146: a neutron. Application of the detai
Page 147 and 148: urning can be treated in such a sta
Page 149 and 150: Currently, all stellar models study
Page 151 and 152: determination of abundance patterns
Page 153 and 154: 4. Scientific Themes 4.5 Fundamenta
Page 155 and 156: This could be achieved at upgraded
Page 157 and 158: experiment that is currently being
Page 159 and 160: ut also scintillating bolometers as
Page 161 and 162: highest experimental sensitivities
Page 163 and 164: New time reversal invariant scalar
Page 165 and 166: due to the interference of photon a
Page 167 and 168: muon intensities. These could be ac
Page 169 and 170: 4.5.4 Properties of Known Basic Int
Page 171 and 172: Highly-charged ions The fourth dire
Page 173 and 174: sponding force acts and α is a str
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Page 178 and 179: 4.6 Nuclear Physics Tools and Appli
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4.6 Nuclear Physics Tools and Appli
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5.1 Contributors Hartmut Abele (Wie
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5.3 Acronyms and Abbreviations ADS
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Published by the European Science F
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