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European Science Foundation Exploratory Workshop How to Constrain the High Density Symmetry Energy HiDeSymE ne European Science Foundation Exploratory.

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Presentation on theme: "European Science Foundation Exploratory Workshop How to Constrain the High Density Symmetry Energy HiDeSymE ne European Science Foundation Exploratory."— Presentation transcript:

1 European Science Foundation Exploratory Workshop How to Constrain the High Density Symmetry Energy HiDeSymE ne European Science Foundation Exploratory Workshop How to Constrain the High Density Symmetry Energy HiDeSymE ne Zoran Basrak September 1, 2010, Egelsbach, Germany Z. Basrak, convenor Strategic Workshop European Science Foundation Standing Committee for Physical and Engineering Sciences Laboratory for Nuclear Physics Division of Experimental Physics Ruđer Bošković Institute, Zagreb, Croatia 1950 – 2010

2 ESF EW HiDeSymEne https://www.irb.hr/users/mkis/

3 Nucleosynthesis

4 Nuclear Equation of state (EoS) p V T pV = nRT SOFT HARD E ( ,I) = E ( ,0) + E sym (  )I 2 + o (I 4 ) +... I = (  n −  p ) /  E sym (  ) ≈ E(  ) neutr. matter - E(  ) sym. nucl. matter

5 Symmetry energy The asymmetry term contributes a greater uncertainty than does the symmetric matter EOS. (Bao-An Li) Z. Xiao et al., PRL 102 (2009) 062502

6 Neutron star  p /  n ≤ 0.1 – 0.2  c ≤ (2-15)  0 J. M. Lattimer and M. Prakash, Phys. Rep. 442 (2007) 109 J. M. Lattimer and M. Prakash, Nucl. Phys. A777 (2006) 479

7 Supra-saturation densities The only available data (FOPI and FOPI–LAND collaborations @ GSI) result in a contradictory predictions for E sym : (Courtesy of M.B. Tsang) Z.Q. Feng, G.M. Jin, PL B683 (2010) 140

8 HiDeSymEne Follow-up activities Follow-up activitiesHiDeSymEne

9 European Science Foundation Research Networking Programmes Constraining the Symmetry EnergyCoSymE European Science Foundation Research Networking Programmes Constraining the Symmetry EnergyCoSymE Z. Basrak, M. Colonna and W. Trautmann

10 How ? GDR & PYGNY RESONANCE

11  Creation of discussion fora: What for ? - new intensive RIB facilities - train up a new generation of scientists to take over leadership  Open character  Exchange of students & experts  Facilitate a global dimension (complementarities)  Timely initiative  Prepare future - theoreticians – experimentalists - nuclear physics – astrophysics

12 Who ? 1Croatia 2France 3Germany 4Italy 5Poland 6Romania 7Spain 8Sweden 9United Kingdom European Science Foundation 30 member states

13 Who ? 1Croatia Department of Physics, University of Split, Split Department of Physics, University of Zagreb, Zagreb Ruđer Bošković Institute, Division of eperimental physics, Zagreb 2France GANIL, CEA/DSM-CNRS/IN2P3, Caen LPC Caen, ENSICAEN, Université de Caen, CNRS/IN2P3, Caen Subatech, EMN-IN2P3/CNRS-Université de Nantes, Nantes Institut de Physique Nucléaire, IN2P3-CNRS, Orsay 3Germany GSI Helmholtzzentrum fur Schwerionenforschung GmbH, Darmstadt FIAS, Universitat Frankfurt, Frankfurt am Main Institute for Theoretical Physics, University of Giessen, Giessen Institute for Theoretical Physics/Astrophysics, University of Heidelberg, Heidelberg 4Italy Dipartimento di Fisica, University of Catania, Catania CSFNSM, Catania INFN – Sezione di Catania, Catania INFN-LNS, Catania Kore University, Enna INFN – Sezione di Milano and Dipartimento di Fisica, Milano INFN – Sezione Napoli and Dipartimento di Fisica, Napoli 5Poland Institute of Physics, University of Silesia, Katowice Faculty of Physics, Astronomy and Applied Computer Science, Jagiellonian University, Krakow IFJ-PAN, Krakow A. Soltan Institute for Nuclear Studies, Swierk/Warsaw Institute of Experimental Physics, Warsaw University, Warsaw Institute for Theoretical Physics, University of Wroclaw, Wroclaw 6Romania NIPNE, Bucharest University of Bucharest and IFIN-HH, Bucharest 7SpainUniversity of Santiago de Compostela, Santiago de Compostela 8Sweden Department of Fundamental Physics, Chalmers University, Göteborg Faculty of Science, Lund University, Lund School of Technology, Malmo University, Malmo 9 United Kingdom STFC Daresbury Laboratory, Warrington, Cheshire University of Liverpool, Liverpool

14 CoSymE proposal assessment

15 Presentations at meetings

16 Lobbying for CoSymE

17 SIS18 ASY-EOS experiment S394 Experiment approved by GSI-PAC ASY-EOS Collaboration Zagreb, Croatia Caen, Orsay, France Darmstadt, Frankfurt, Germany Ioannina, Greece Catania, Milano, Napoli, Italy Katowice, Krakow, Warsaw, Poland Bucharest, Romania Santiago de Compostela, Spain Lund, Malmo, Sweden Daresbury, Liverpool, United Kingdom Kolkata, India NSCL-MSU, Rochester, USA GSI LAND LNS Chimera.5 m Lund-SdC Califa IPJ phoswich MSU miniball

18 European Science Foundation Exploratory Workshop How to Constrain the High Density Symmetry Energy HiDeSymE ne European Science Foundation Exploratory Workshop How to Constrain the High Density Symmetry Energy HiDeSymE ne Zoran Basrak September 1, 2010, Egelsbach, Germany Z. Basrak, convenor Strategic Workshop European Science Foundation Standing Committee for Physical and Engineering Sciences Laboratory for Nuclear Physics Division of Experimental Physics Ruđer Bošković Institute, Zagreb, Croatia 1950 – 2010 Thank you for your attention


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