Perspectives of Nuclear Physics in Europe - European Science ...

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For more information contact: Professor Günther Rosner NuPECC Chair School of Physics and Astronomy University of Glasgow University Avenue Glasgow G12 8QQ United Kingdom Tel: +44 141 330 2774 Fax: +44 141 330 2630 Email: g.rosner@physics.gla.ac.uk Dr Gabriele-Elisabeth Körner NuPECC Scientific Secretary c/o Physik-Department E 12 Technische Universität München 85748 Garching Germany Tel: +49 89 2891 2293 Fax: +49 89 2891 2298 Email: sissy.koerner@ph.tum.de www.nupecc.org Physical and Engineering Sciences Unit European Science Foundation 1 quai Lezay-Marnésia BP 90015 67080 Strasbourg cedex France Tel: +33 3 88 76 71 00 Fax: +33 3 88 37 05 32 Email: pesc@esf.org or lrp2010@esf.org www.esf.org Print run: 1 000 – December 2010
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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
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concentrate their efforts and conti
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4. Scientific Themes 4.2 Phases of
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tion of state would therefore deter
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an increase at the deconfinement te
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can be described with statistical h
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Box 3. Heavy ion fragmentation and
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Figure 7. Isotopic dependence of th
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energies so far did not find indica
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4.2.5 The High-Energy Frontier The
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Figure 10. Elliptic flow parameter
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elevant experimental and analysis r
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the same time being able to precise
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technology), a three-dimensional ar
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4. Scientific Themes 4.3 Nuclear St
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4.3.2 Theoretical Aspects Ab Initio
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the continuum, as done, e.g., in th
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Each of these extensions will open
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Halos, clusters and few-body correl
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Figure 3. Mirror Energy Differences
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Superheavy elements The existence o
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Figure 5. Gamma-ray spectrum of the
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The experimental evidence for the e
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4.3.7 Ground-State Properties Figur
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For nuclear astrophysics applicatio
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A detector array for high-energy ph
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and rejection power of separators.
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4. Scientific Themes 4.4 Nuclear As
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powers many of the objects we obser
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Hydrostatic burning Stars spend the
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Significant uncertainties remain fo
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nova ejecta (a few seconds). In thi
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have to be calculated. Current micr
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An improvement in the precision of
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a neutron. Application of the detai
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urning can be treated in such a sta
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Currently, all stellar models study
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determination of abundance patterns
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4. Scientific Themes 4.5 Fundamenta
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This could be achieved at upgraded
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Page 159 and 160: ut also scintillating bolometers as
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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
Page 203 and 204: 5.1 Contributors Hartmut Abele (Wie
Page 205 and 206: 5.3 Acronyms and Abbreviations ADS
Page 207: Published by the European Science F
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