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

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5.3 Acronyms and Abbreviations JRA joint research activity JYFL Univertiy of Jyväskylä KVI Kernfysisch Versneller Instituut LCB laser Compton backscattering LEAR Low Energy Antiproton Ring LEO low earth orbit LET linear energy transfer LHC Large Hadron Collider LHeC Large Hadron electron Collider LNGS Laboratory Nazionali di Gran Sasso LNL Laboratori Nazionali di Legnaro LNS Laboratori Nazionali del Sud LNT linear-no-threshold LQCD lattice QCD LUNA Laboratory Underground for Nuclear Astrophysics MAMI Mainz Mikrotron MAPS monolithic active pixel sensors MC Monte Carlo MPGD micro-pattern gas detectors MRI magnetic resonance imaging NA49 North Area, CERN, Experiment 49 NCSM no-core shell model NIF National Ignition Facility NIST National Institute of Standards and Technology NuSTAR Nuclear Structure, Astrophysics and Reactions PANDA antiProton ANnihilation at DArmstadt PARIS Photon Array for studies with Radioactive Ion and Stable beams PAX Polarized Antiproton eXperiments PET positron emission tomography PHELIX Petawatt High Energy Laser for heavy Ion eXperiments PSI Paul-Scherrer-Institut PVeS parity-violating electron scattering QCD quantum chromodynamics QED quantum electrodynamics R3B Reactions with Relativistic Radioactive Beams RBE relative biological effectiveness RHIC Relativistic Heavy Ion Collider RPA random phase approximation SEE single event effect SEU single event upset SHE superheavy elements SLAC Stanford Linear Accelerator SM standard model or shell model SMMC SN SNM SPE SPECT SPES SPIRAL SUSY TASCA THM TMD TNA TOF WD WEP shell-model Monte Carlo supernova special nuclear material solar particle events single-photon emission computerized tomography Selective Production of Exotic Species Système de Production d’Ions Radioactifs Accélérés en Ligne supersymmetry TransActinide Separator and Chemistry Apparatus Trojan horse method transverse momentum dependent distribution function transnational access time of flight white dwarf weak-equivalence principle 204 | Perspectives of Nuclear Physics in Europe – NuPECC Long Range Plan 2010
Published by the European Science Foundation November 2010 Printing: IREG, Strasbourg ISBN: 978-2-918428-29-9
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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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Page 159 and 160: ut also scintillating bolometers as
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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: 5.3 Acronyms and Abbreviations ADS
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