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  Interfaces between Structure and Reactions for Rare Isotopes and Nuclear Astrophysics 
 
  
 The goal of this INT
                Program was to identify those problems in the area of
                theory for reactions with rare isotopes that need to be
                solved in order to plan experiments for FRIB (the
                Facility for Rare Isotopes) and in order to understand
                the experimental results in terms of nuclear structure
                and applications to nuclear astrophysics. The program
                brought together reaction and structure theorists who
                worked together to identify specific needs of reaction
                theory and propose paths for their solutions and
                implementation. The Program was
                preceded by the 7th ANL/JINA/MSU annual FRIB workshop on
                "Interfaces between Nuclear Reactions and Structure"
                which was held from August 8-12, 2011 [Organizers B. A.
                Brown (Chair), P. Danielewicz, G. F. Bertsch]. The
                talk-intensive workshop had a large input from
                experimentalists, who were encouraged to formulate
                charges and challenges to nuclear structure and reaction
                theory that could both influence and benefit
                experimental nuclear physics research programs. The
                experimental talks included the topics of one-nucleon
                transfer and knockout reactions; two-particle transfer,
                two-particle knockout and two-particle decay;
                charge-exchange reactions and their connections to
                nuclear astrophysics; and medium to high energy
                heavy-ion reactions. Discussions included: What is the
                role of nuclear correlations on the one-particle
                transfer form factors. What is the role of pairing (T=1)
                and proton-neutron (T=0) correlations on reaction and
                structure observables? What constraints can be put on
                the nuclear equations of state? What improvement are
                required for the reaction theory codes that are used to
                interpret the data? The pictures below give some
                examples from the talks of Wilton Catford and Remco
                Zegers on the new detector systems being used.  The
                Program consisted of seminars, group discussions and
                many one-on-one interactions. Group discussions included
                the topics of (1) making computer codes available to the
                practitioners, (2) the validity of the eikonal
                approximation, (3) the problems of center-of-mass motion
                in nuclear structure and reactions, (4) the nature of
                the Hoyle state in 12C, (5) time-dependent reaction
                models and (6) fusion models.   The
                talks focusing on reactions included the topics of
                coupled channels CDCC methods for light-ion reactions,
                coupled channels methods for sub-barrier fusion, models
                for radiative capture and Coulomb excitation for nuclei
                near the drip lines, time-dependent Hartree-Fock methods
                for heavy-ion fusion, applications of the dispersive
                optical model for one-nucleon overlap functions, and
                transport and quantum hydrodynamics models for
                intermediate energy reactions.  
  (INT Workshop August 8 - September 2, 2011)
    Reported by B. A.  Brown (chair), H. Esbensen, P. Danielewicz and J.A. Tostevin
  Date posted November 9, 2011
 
  
     
  
  
        
                
                
                
                 
   
              
                
                
              
                
                
                Theoretical talks were spread over the Workshop and the
                Program. The talks focusing on nuclear structure
                included the topics of ab-initio theory for light
                nuclei, many-body methods that include the continuum,
                the dependence of the overlap functions on the energy
                scale of the theory, mean-field models including T=1
                pairing for the nuclear ground state, time-dependent
                mean-field approaches for nuclear excited states. The
                pictures below give some examples from the talks of Petr
                Navratil and Gaute Hagen on the theoretical formulations
                being used.
                
              
              
   
              
                
                
                
                
                As an outcome of the Program, the organizers and
                participants have contributed to a white-paper that
                outlines in detail the specific needs for improvements
                in reaction theory and related reaction theory computer
                codes. The participants also agreed to support a website
                where the commonly used computer codes and documentation
                could be accessed by the theoretical and experimental
                practitioners.
                
                The Workshop and Program were successful in illuminating
                the theoretical problems that need to be solved for
                understanding the rich nuclear landscape from stable to
                neutron-rich nuclei (below left), and their implications
                for nuclear astrophysics such as the properties of
                neutron stars (below right).
                
              
                
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