1. Current status and future direction on symmetry energy determination using Heavy Ion Collisions How does this subfield intersect with other subfields? Betty Tsang Nuclear Astrophysics town meeting October 8-10, 2012 Detroit, Michigan Neutron Stars and Dense Matter Working Group

2. Current status and future direction on symmetry energy determination using Heavy Ion Collisions Graffiti Art, Dequindre Cut, Detroit, August, 2012 Artist: Kobie Solomon How does this subfield intersect with other subfields?

3. EoS of asymmetric matter E/A ( ,  ) = E/A ( ,0) +  2  S(  )  = (  n -  p )/ (  n +  p ) = (N-Z)/A  1 The symmetry energy influences many properties of neutron stars: –Radii, moments of inertia –Cooling rates –Phase transitions in interior The symmetry energy dominates the uncertainty in the n-matter EOS. B.A. Brown,PRL85(2000)5296 Tsang et al,PRL102,122701(2009) Constraints from Heavy Ion Collisions (HIC) major recent accomplishments

4. Tsang et al. C 86, 015803 (2012) HIC: heavy ion collisions; PRL 102,122701(2009) p elastic scattering PRC82,044611(2010) Isobaric Analogue States NPA 818, 36 (2009) neutron-star radius PRL108,01102(2012) Pygmy Dipole Resonances PRC 81, 041304 (2010) Finite Droplet Range Model PRL108,052501(2012) Consistent Constraints on Symmetry Energy from different experiments  HIC is a viable probe major recent accomplishments How does this subfield intersect with other subfields

5. Summary of 208 Pb n-skin thickness constraints Model calculations with and without 3nn forces: BHF: PRC80,045806 (2009) Brueckner-Hartree-Fock DBHF: arXiv:1111.0695 Dirac Brueckner-Hartree-Fock CEFT :PRL105,161102(2010) Chiral Effective Field Theory QMC :PRC85,032801R(2012) Quantum Monte Carlo Importance of 3-body neutron-neutron force in the Equation of State of pure neutron matter Tsang et al.PRC (in print) arXiv:1204.0466 neutron star major recent accomplishments

6. Effective nucleon masses At  <  0 density, effect of mass splitting increases with density and asymmetry Zhang, private communications specific compelling open questions Coupland et al

7. FAIR  RIBF’12, FRIB’20,RISP? GSI’11 Symmetry Energy Project: International collaboration to determine the symmetry energy over a range of densities How can one address these open questions?

8. high impact nuclear experiments Symmetry Energy Project: International collaboration to determine the symmetry energy over a range of densities facilityProbe Beam Energy (A MeV) yeardensity MSUn, p,t,3He50-1402009 <o<o GSIn, p, t, 3He4002011 2.5  o MSUiso-diffusion502011 <o<o RIKENiso-diffusion502013 <o<o MSU +,-+,- 1402014-2015 1-1.5  o RIKEN n,p,t, 3 He,  +,  - 200-3002013-2014 2o2o GSIn, p, t, 3He8002014 2-3  o FRIB n,p,t, 3 He,  +,  - 2002018- 2-2.5  o

9. 124 Sn+ 124 Sn E lab =120 MeV/A b = 1fm BUU from: Danielewicz, NPA673, 375 (2000). New observables:  - /  + ratio New detectors: SAMURARI- Time Projection Chamber Active Target -Time Projection Chamber To probe symmetry energy at  >  0 with sub-threshold pions from HIC Bickley et al., private comm. (2009) B.A. Brown,PRL85(2000)5296 Tsang et al,PRL102,122701(2009) specific compelling open questions

10. MSU Active Target-Time Projection Chamber Cathode Corona Ring Beam Beam tube Field Cage Micromegas GET electronics Properties of AT-TPC Length 1 m. Diameter 0.7 m 10000 Pad Self-triggering electronics How can one address these open questions?

11. MSU Active Target-Time Projection Chamber 130 cm 70 cm Lead PI :W. Mittig; Project leader: D. Bazin; Co-PI: W. Lynch AT-TPC will allow inverse kinematics studies in astrophysical, resonant, transfer, breakup, fusion, fission reactions and to study the EOS using giant resonances and heavy ion reactions. AT-TPC will make use of the full range of beam energies and intensities available from ReA3 and FRIB. Half-size proto-type is working Broad innovative scientific program. Two alternate modes of operation Fixed Target Mode with solid target inside chamber: –4  tracking of charged particles allows full event characterization Active Target Mode: –Chamber gas acts as both detector and target ( H 2, D 2, 3 He, Ne, etc.) –Provides a thick target for low intensity beams while retaining high resolution and efficiency high impact nuclear experiments

12. Time-projection chamber (TPC) will sit within SAMURAI dipole magnet Auxiliary detectors for heavy-ions and neutrons, and trigger Hodoscope Nebula (neutron array) SAMURAI dipole magnet and vacuum chamber SAMURAI-TPC beam slide courtesy of R. Shane SAMURAI-TPC (2014) How can one address these open questions?

13. DISCUSSION POINTS 1. What are the major recent accomplishments? constraints at subsaturation density 2. What are the specific compelling open questions? (Unexplained observations, problems in theoretical modeling, etc.)  /  0 >1: S(  ); effective nucleon masses, effect of 3n forces in EOS 3. How can one address these open questions? What are the high impact nuclear experiments, observations, theoretical studies that need to be done? $; new detectors; FRIB (high intensity RIB); improved theories 4. In which direction should this area evolve in light of expected new observational, theoretical, and experimental capabilities? exploration of  /  0 > 1 and  /  0 <<1; understanding of basic physics properties of nuclear matter (m*). 5. How does this subfield intersect with other subfields? (For example, is there work needed in other subfields to move this subfield forward). Improvement in transport theories; neutron star observations;