Hirschegg Workshop 2008
Abstracts


Lastname, Firstname Title
Abstract
 
Aliotta, Marialuisa Radioactive beams for astrophyics: recent studies and open questions
The talk will present an overview of some recent experimental studies relative to explosive nuclear burning in astrophysical scenarios such as novae and X-ray bursts. Current status and open questions will also be discussed.
 
Badarch, Urnaa
Density dependence of the symmetry energy.
One of the major puzzles of modern nuclear many-body theory is the density dependence of the symmetry energy. The variation of the symmetry energy with total density is of high importance for a large variety of phenomena ranging from fragmentation in high energy heavy ion reactions to the structure of neutron stars. Despite many experimental and theoretical attempts there are remaining uncertainties leaving open questions. We use DDRH field theory to investigate the symmetry energy, the compressibility, and other thermodynamical quantities of nuclear matter over a large density range on a fully microscopic level. Since we use interaction from Dirac-Brueckner theory our approach is well defined in a diagrammatically sense. The special role of the delta-($a_0(980)$) meson for the effective masses is discussed. The DDRH approach allows a fully self-consistent derivation of the equation of state and the symmetry energy at any proton-to-neutron fraction. A comparison of the DDRH results to those from phenomenological approaches shows significant deviations at very low and high densities relevant for neutron star calculations. The effects on neutron star matter in beta-equilibrium are discussed. Results for the mass-radius relation, i.e. the equation of state of neutron stars are discussed.
 
Barbieri, Carlo Applications of Green's function techniques to nuclear structure (and atoms)
The talk will cover recent ab-initio calculations of the Faddeev expansion method to both nuclei and light atoms. For atoms, the Faddeev-RPA approximation has been found to match the best calculations of ionization energies and strengths (corresponding to separation energies and spectroscopic factors in nuclear physics). First calculations for nuclei will be reported. The relevance of this method to the the study of transfer reactions and nuclear response will be discussed.
 
Blank, Bertram Tow-proton radioactivity studies
I will present an overview of present and past two-proton radioactivity studies. Experimental results will be compared to theoretical predictions and new experimental developments will be described.
 
Boretzky, Konstanze Pygmy Dipole Strength in Exotic Nuclei and the Neutron Equation of State
The properties of exotic nuclei are ideally studied in inverse-kinematics experiments at high beam energies using the FRS-LAND facilities at GSI, allowing exclusive measurements of all projectile-like particles following the excitation of the projectile in a high-Z target (Pb). At beam energies of ~500 MeV/u electromagnetic excitations are dominated by dipole transitions. In an experiment utilizing secondary beams of neutron-rich Sn isotopes $^{129-132}$Sn and neighbouring nuclei with similar A/Z ratio a substantial fraction of dipole strength at energies below the giant dipole resonance (GDR) is observed. For $^{130}$Sn and $^{132}$Sn this strength is located in a peak-like structure around 10 MeV and exhibits a few percent of the Thomas-Reiche Kuhn (TRK) sum-rule strength. Several calculations predict the appearance of dipole strength at low excitation energies in neutron-rich nuclei, often referred to as pygmy dipole resonance (PDR). In a macroscopic picture, the PDR is discussed in terms of a collective oscillation of excess neutrons out of phase with the core nucleons. Recent random-phase-approximation calculations show a strong correlation of the PDR strength to the density dependence of the symmetry energy and thus a link to the neutron skin size. Consequences from the experimental findings in $^{130}$Sn, $^{132}$Sn and $^{208}$Pb for the neutron-skin sizes, the symmetry energy and the neutron equation of state (EoS) will be discussed.

Brown, Alex Hybrid Methods for Nuclear Structure
 I will review some recent results for shell-model configuration mixing and Skyrme Hartree-Fock calculations for nuclei in the region A=20-60, and review the strong and weak aspects of each method. Hybrid methods involve making use of the best aspects of both methods, together with input from renormalized NN interactions.

Brunner, Thomas Measurements of Electron Capture Branching Ratios at the TITAN Ion Trap Facility to Evaluate Double-Beta Decay Nuclear Matrix Elements
The TITAN (TRIUMF's Ion Traps for Atomic and Nuclear physics) trap system is a new facility whose primary application is high-precision atomic mass measurements on short-lived radio-nuclides. Mass measurements are performed with a Penning-trap mass spectrometer in combination with an EBIT (Electron Beam Ion Trap), which is used as a charge breeder to enhance the precision of mass measurements. The EBIT offers the possibility to measure nuclear-decay electron capture branching ratios (ECBRs) on stored radio-active ions through X-ray spectroscopy. With no electron beam, the EBIT traps ions with electrostatic potentials applied to drift tubes and a strong magnetic field provided by two coils in the Helmholtz configuration giving a visible access to the trap center. In comparison to conventional techniques, the advantage of an ion trap is the backing free storage of ions and thus a lower background. The EBIT, combined with the wide range of radioactive isotopes supplied by TRIUMF's ISAC facility, offers a novel approach to measure ECBRs for odd-odd intermediate nuclei involved in double-beta decay ($\beta^-\beta^-$). In the neutrinoless $\beta\beta$ decay, the neutrino mass is a function of the nuclear matrix elements and the transition probability. If $0\nu\beta\beta$ decay is observed in experiments such as NEMO, Majorana and EXO, ECBRs can be used to obtain a detailed knowledge on the transition nuclear matrix elements from which the neutrino mass can then be evaluated.
 
Enders, Joachim Polarized Electrons at Low Momentum Transfers - Technical Developments and Planned Experiments at the S-DALINAC
For future use at the superconducting Darmstadt electron linear accelerator S-DALINAC, a source of polarized electrons is being developed and tested, first as an offline test stand. Longitudinally polarized photo-electrons are produced using a pulsed diode laser and GaAs photo-cathodes and are preaccelerated electrostatically to 100 keV. First measurements of beam parameters as well as the status of technical developments will be discussed. Furthermore, planned experiments with polarized electron and photon beams at low energies and momentum transfers will be presented. First tests (with unpolarized beams) searching for parity-violation effects in photo-induced fission have already been performed. Electron scattering experiments on light nuclei are foreseen to elucidate the role of, e.g., mesonic exchange currents and of the three-body force in few-body systems.
 
Gade, Alexandra Nuclear spectroscopy with fast exotic beams
 
 
Geissel, Hans Experiments with stored exotic nuclei with FRS-ESR
 
 
Herfurth, Frank Ion traps and nuclear spectroscopy
Ion trap setups like SHIPTRAP, ISOLTRAP or the planned MATS facility provide clean and well-controlled samples of short-lived nuclei. This is an ideal prerequisite for nuclear decay spectroscopy either using the backing free, well localized sample in the trap or the high mass resolving power and long storage times of a Penning trap for spectroscopy after the trap. Demonstration experiments have been performed on a number of trap setups and will be presented. In addition, this presentation focuses on future experiments for instance at the MATS setup at FAIR or TRIGA-Trap at the research reactor in Mainz. Detailed alpha spectroscopy will be used to measure the lifetime of excited nuclear states for the determination of, for instance, quadrupole moments of 2+ states. The electrons shaken off from the recoil will be extracted out of the magnetic field and deliver the position information from the alpha decay and the subsequent electron conversion decay and hence the lifetime of the state populated by the first decay.
 
Herlert, Alexander The HIE-ISOLDE Project
Forty years after ISOLDE started operation at CERN in 1967 it is still today the leading ISOL facility in terms of the variety of extracted radioactive beams. An increasingly important component during the last years has been the REX-ISOLDE post-accelerator that presently can accelerate most ion beams produced at ISOLDE up to a maximum energy of 3 MeV/u. The HIE-ISOLDE project includes several important upgrades of the present facility. The existing post-accelerator will be extended with an intermediate step with acceleration to 5.5 MeV/u and the final objective being to provide radioactive beams up to 10 MeV/u. For the extension superconducting technology will be used. The beam quality will be improved in several respects: through the installation of an RFQ cooler, a new resonant laser ionization system, and a renovated High Resolution Mass Separator. Combined with the continuing target and ion source developments this will provide significant improvements for experiments and give a total of more than 1000 different ISOL beams. Finally, the driver beam intensity will be increased, at first due to a faster cycling of the PS Booster accelerator, at a later stage due to the new injector accelerator Linac-4. The target design will be adapted to accommodate this higher intensity. The presentation will focus on the technical improvements and will give selected examples of the physics possibilities that will emerge as the different parts of the project are implemented.
 
Higa, Renato alpha-alpha scattering within Halo EFT
Recently, rare exotic nuclei have drawn a lot of interest due to properties that challenge traditional knowledge gained from studies of stable nuclei. Particularly interesting is the formation of clusters and halo structures, whose small bindings lead to threshold phenomena with important consequences for nuclear astrophysics. In many cases the binding among clusters is much smaller than the exitation energy of each separate cluster, making them suitable systems for employing Effective Field Theory (EFT) techniques. Halo EFT has been developed and successfully applied to neutron-alpha scattering, with a proper account of the $P_{3/2}$ resonance around 1 MeV. However, in many systems Coulomb interactions play a significant role, therefore an extension which incorporates these effects is highly desirable. I will present such an extension, based on previous works by Kong and Ravndal, with application to low-energy alpha-alpha scattering.
 
Holt, Jason Low Momentum Interactions for Nuclear Structure
This talk will focus on presenting recent results and future prospects of a theoretical program which aims to use low-momentum interactions to describe nuclear structure properties of medium-mass nuclei. Using two-nucleon (NN) low-momentum interactions $V_{{\rm low}\,k}$, we study collective isovector valence shell excitations (mixed-symmetry states) of nuclei in the mass A=90 region. I will discuss the insights we gain into the underlying mechanisms driving the formation and evolution of these structures in the N=52 isotones and emphasize the close connection this work has with recent experimental investigations such as g factor measurements and electron- and proton-scattering cross sections. Variations in the NN-interaction-only results with the resolution/cutoff scale suggest the need for many-body forces, and I will discuss the first steps taken to incorporate three-nucleon interactions in this program.
 
Karasu Uysal, Ayben Isovector Dipole Excitations in Hot Nuclear Matter
We study the isovector dipole excitations in nuclear matter by employing the linearized Landau-Vlasov equation at finite temperature using Skyrme and Gogny forces for infinite nuclear matter and Skyrme force, Gogny force and Landau-Migdal interaction for finite nuclei in semiclassical Thomas-Fermi approximation. We calculate the giant dipole resonance (GDR) strength function for these cases for 120Sn and 208Pb and compare our results.
 
Kowalska, Magdalena Structure of light nuclei derived from their ground-state properties: masses, spins, moments, radii.
Light nuclei host a variety of intriguing nuclear phenomena: They form halos, clusters, or molecular structures, where the latter very often correspond to strongly deformed shapes; the effect of a magic numbers seems to erode to the point of disappearance, as is the case for the 'island of inversion' around N=20. Several modern theoretical approaches successfully describe these properties: cluster models, ab initio calculations (available up to A=10), or new shell model approaches, such as the Monte Carlo or no-core shell model. In order to test and refine these theoretical descriptions of the few-nucleon systems, the corresponding experimental observables have to be available, and the nuclear ground-state properties: masses, spins, magnetic and electric moments, and charge radii, represent such model-free observables. In this talk I will present recent obtained with two experiments located at ISOLDE/CERN: high-precision Penning trap mass spectrometer ISOLTRAP and collinear laser-spectroscopy and beta-NMR setup COLLAPS. These results include mass, magnetic moment, and charge radius of the proton halo candidate $^{17}$Ne, which characterize the main components of its ground-state configuration. The magnetic and quadrupole moments of $^{9,11}$Li, which determine to which extend $^9$Li core stays inert in $^{11}$Li will be also discussed. Finally, I will present spins and magnetic moments of $^{29,31,33}$Mg, which help to determine the physics mechanism driving the 'island'.
 
Krücken, Reiner Probing Shell closures and shape coexistence with MINIBALL
In this contribution selected recent results on spectroscopic investigations with the MINIBALL Gamma-ray spectromter will be presented. On one hand results from Coulomb-excitation and first transfer experiments at REX-ISOLDE will discussed, which concern the investigation of shell evolution and shape coexistence. Particular examples concern results at the boarder of the island of inversion, near the doubly magic nuclei $^{78}$Ni, $^{132}$Sn, as well as first Coulex experiments in the A=200 mass region. In addition results from a knock-out experiment at the GSI Fragment Speparator with MINIBALL will be presented. The results allow for the first time a clear determination of the ground state spin in $^{55}$Ti as well as occupation probabilities of the relevant single-particle states. The results will be compared to modern shell model calcultations.
 
Lenske, Horst Relativistic Density Functional Theory
The DDRH theory as a fully covariant and thermodynamically consistent density functional field theory is used to investigate the dynamical structure of in-medium NN interactions. In-medium NN interactions are obtained from Dirac-Brueckner calculations. The interaction vertices are treated on the level of the Lagrangian as Lorentz-scalar functionals of the field operators. Results for the equation of state of infinite nuclear matter, hypermatter, and neutron starts are discussed. Binding energies of finite nuclei are well reproduced on a level of accuracy of a few percent. In order to achieve a better understanding of density dependent effects, we investigate their contribution to dynamical scenarios involving excitations at non-vanishing energy and momentum transfer. We choose Landau's Fermi-liquid theory and extend the approach to relativistic density functionals. In order to retain the field theoretical structure we derive the interaction functional in a general from by second variation with respect to the field operators. The Landau-Migdal-Parameters are obtained by expanding the interaction amplitudes around the ground state expectation value. We analyze the impact of rearrangement effects in the quasiparticle interaction, which always occur in a density dependent formalism. An important feature is the remarkable modification of the variationally derived Landau-Migdal interaction in asymmetric matter by isovector effects due to the neutron excess.
 
Maris, Pieter Recent advances in ab initio calculations of nuclear structure
I discuss recent developments in "ab initio" calculations of nuclear structure using basis function expansion methods. In principle any nuclear potential can be used as input for such calculations, though numerical convergence depends on the softness of the potential. Renormalizations methods such as Lee-Suzuki and similarity group transformations have been used to improve convergence. Our calculations with chiral effective two-nucleon and three-nucleon potentials and with a phenomenological two-body potential (JISP16) give a good description of a range of properties of light nuclei.
 
Neff, Thomas Structure and reactions of light nuclei in the Fermionic Molecular Dynamics approach
Light nuclei show a wealth of exotic phenomena like clustering and halos. We aim at a consistent description of light nuclei in the Fermionic Molecular Dynamics (FMD) approach, a microscopic many-body model that uses Slater determinants built with Gaussian wave packets as basis states. We employ an effective interaction derived from the realistic Argonne V18 interaction by explicitly implementing shortrange central and tensor correlations using the Unitary Correlation Operator Method. We will show results for nuclei in the p- and sd-shell, looking at binding energies, spectra, charge and matter radii, electromagnetic and weak transitions. The FMD wave functions can be analyzed with respect to clustering and shell model occupations. The structure of 12C will be analyzed in detail with a special emphasis on the Hoyle and other cluster states. The implementation of resonance and scattering boundary conditions also allow us to study low-energy nuclear reactions like the radiative capture reaction 3He(alpha,gamma )7Be.
 
Nogga, Andreas Using light nuclei to probe chiral nuclear interactions
Chiral perturbation theory is a promising approach to systematically develop nuclear interactions. For this endeavor the light nuclei are especially interesting laboratories since they are specifically sensitive to subleading parts of the interactions, e.g. three-nucleon interactions. In this talk, I will review recent results for nuclear bound states based on chiral interactions and discuss their implications for further developments of chiral interactions.
 
Nowacki, Frederic
Shell evolution far from stability in the (sd-pf) region


Orrigo, Sonja Correlation effects and continuum spectroscopy in light exotic nuclei
The spectroscopy of exotic nuclei is one main topic of modern nuclear structure physics. Unexpected phenomena have been observed in light n-rich nuclei. The enhanced correlation dynamics makes possible new continuum excitation modes, the Fano Resonances, a class of states above the neutron emission threshold due to dynamical core polarization effects, characterized by asymmetric line shape. By the Quasiparticle-Core Coupling model we show that the coupling of 1QP and 3QP core-excited components leads to sharp resonances in the low-energy continuum of the n+core system, with interference effects. Theoretical calculations are presented for $^{15}$C, $^{17}$C and $^{19}$C, giving information on the evolution of the phenomenon with the neutron excess. The comparison with the $^{15}$C experimental data shows a very good qualitative agreement. Differently from well bound stable nuclei, in weakly bound n-rich nuclei the relevant energy scale is given by the separation energy of valence particles (few hundreds of keV). Thus interactions down this order of magnitude have to be included, such as pairing effects, which are complementary by creating a genuine type of configuration mixing already at the mean-field level. Single-nucleon transfer reactions are investigated as tool for continuum spectroscopy in nuclei such as $^{10}$Li. We present a DWBA approach which allows to treat the case of unbound final states, applied to the $^{9}$Li(d,p) $^{10}$Li reaction at 3 and 20 MeV/u.
 
Paar, Nils Inclusive neutrino-nucleus cross sections based on the relativistic mean-field theory
Inclusive neutrino-nucleus cross sections are studied within consistent relativistic mean-field theoretical framework. The weak lepton-hadron interaction is expressed in the standard current-current form, the nuclear ground state is described with the relativistic Hartree-Bogoliubov model, and the relevant transitions to excited nuclear states are calculated in the relativistic quasiparticle random phase approximation. Illustrative test calculations are performed for charged-current neutrino reactions on $^{12}$C, $^{16}$O, $^{56}$Fe, and $^{208}$Pb, and results compared with previous studies and available data. Using the experimental neutrino fluxes, the averaged cross sections are evaluated for nuclei of interest for neutrino detectors. We analyze the total neutrino-nucleus cross sections, and the evolution of the contribution of the different multipole excitations as a function of neutrino energy. It is shown that the knowledge on spin-dipole and excitations of higher multipolarities is of outmost importance for reliable microscopic description of neutrino-nucleus reactions. The cross sections for reactions of supernova neutrinos on $^{16}$O and $^{208}$Pb target nuclei are analyzed as functions of the temperature and chemical potential.
 
Pakarinen, Janne Competing structures in light Pb nuclei; extending in-beam gamma-ray measurements to odd-mass Pb isotopes
In very neutron deficient Pb isotopes, both experimental and theoretical evidence for shape coexisting configurations has been achieved [1,2]. This phenomenon becomes transparent particularly at the neutron midshell, where the competing structures intrude down to energies close to the spherical ground state. Together with the spherical ground state, they form a unique triplet of 0$^{+}$ states in $^{186}$Pb, each of which can be associated with a different shape [3]. However, no unambiguous evidence regarding their shape has been achieved in in-beam experiments. To probe this, one could, for example, study rotational coupling in the odd-mass Pb isotopes. In a recent in-beam recoil-decay tagging experiment at JYFL, we have observed excited states in $^{185}$Pb for the first time. In this experiment we collected gamma-gamma-coincidence data that enabled us to construct a level scheme on top of the 13/2$^{+}$ alpha decaying isomeric state in $^{185}Pb. It reveals a band structure which clearly represents strong coupling of an odd i$_{13/2}$ neutron to a prolate core. The interpretation of these new findings will be discussed with respect to the shape coexistence phenomena in light Pb isotopes. [1] J.L. Wood et al., Phys. Rep. 215, 101 (1992). [2] R. Julin, K. Helariutta and M. Muikku, J. Phys. G: Nucl. Part. Phys. 27, R109 (2001). [3] A.N. Andreyev et al., Nature, 405, 430 (2000).
 
Papakonstantinou, Panagiota Giant Resonances with Correlated Realistic Interactions and Second RPA
Second RPA (SRPA) has been applied to study giant resonances (GRs) of closed-shell nuclei. A correlated realistic interaction, constructed within the Unitary Correlation Operator Method (UCOM) so as to take into account short-range correlations, is used to describe the Hartree-Fock (HF) ground state and the residual couplings. It is found, that the second order configurations included in SRPA produce sizable effects, compared to first-order RPA, by effectively dressing the underlying HF single-particle states with self-energy insertions. The effect appears essential for a realistic description of the isovector dipole and isoscalar quadrupole GRs, when using UCOM-correlated interactions. Self-consistency issues of SRPA and the role of missing three-body effects are discussed.
 
Papenbrock, Thomas F. Coupled-cluster theory for nuclei
I will give an overview of ab-initio nuclear structure calculations based on coupled-cluster theory. The focus will be on recent results obtained for weakly bound and unbound Helium isotopes, the treatment of three-nucleon forces, and the extension to medium-mass nuclei.
 
Quaglioni, Sofia Ab initio nuclear reactions within the NCSM/RGM approach
We report on recent results of our work in the direction of building an {\em ab initio} method for low-energy light-ion reactions by augmenting the no-core shell model (NCSM)$^{1,2}$ to include clustering and resonant and non-resonant continuum. For this purpose, we adapt the resonating group method$^{3}$, a microscopic technique in which the many-body problem is mapped onto various channels of nucleon clusters and their relative motion. In our approach we use NCSM wave functions for the clusters involved, and NCSM effective interactions derived from realistic interactions. In particular, we will present our first results for the scattering of low-energy neutrons on $^4$He. This work was performed under the auspices of the U. S. Department of Energy by the University of California, Lawrence Livermore National Laboratory under contract No. W-7405-Eng-48. Support from U.S. DOE/SC/NP (Work Proposal Number SCW0498) is acknowledged.\\ {\bf References }\\ 1. P.~Navr{\'a}til et al, Phys. Rev. Lett. {\bf 84}, 5728 (2000); Phys. Rev. C {\bf 62}, 054311 (2000).\\ 2. P.~Navr{\'a}til and W.~E. Ormand, Phys. Rev. Lett. {\bf 88}, 152502 (2002); Phys. Rev. C {\bf 68}, 034305 (2003).\\ 3. K.~Wildermuth and Y.~C.~Tang , A Unified Theory of the Nucleus., Vieweg, Braunschweig (1977).
 
Ring, Peter Covariant density functional theory and description of excited states in nuclei far from stability
Covariant density functional theory is used to describe excited states in nuclei far from stability. First we stay in the concept of the mean field approximation and discuss new results obtained in the framework of relativistic quasiparticle RPA (RQRPA) in deformed nuclei. In particular we report on the E1-strength distributions in chains of Ne and Mo isotopes, which have been investigated recently at GANIL and in Rossendorf, and on low the lying M1-strength in nuclei with large neutron excess. Besides the conventional scissor mode, where protons and neutrons occillate against each other, a new mode is found in these calculation, where the neutron skin oscillates in a scissor like motion against the deformed core of protons and neutrons moving in phase. In a second step we go beyond the mean field approximation and discuss recent applications of the relativistic Generator Coordinate Method (GCM) in transitional nuclei.
 
Ringle, Ryan Towards a Penning Trap Mass Measurement of {11}^Li
The halo structure of certain nuclei, such as {11}^Li, is currently one of the most interesting phenomena observed far from stability. It is not only interesting from a nuclear structure point of view, but serves as an example of quantum behavior in a microscopic few-body system, where some of its weakly bound components tunnel beyond the binding potential of the core. Since the first experiments in 1985 which implied a large matter radius, copious amount of effort, both experimental and theoretical, has been expended in understanding the halo nature of {11}^Li (and other halo nuclei). The S_{2N} value of {11}^Li is a key ingredient in models attempting to describe halo structure. The newly commissioned TITAN facility at TRIUMF is ideal for making a Penning trap mass measurement of {11}^Li.
 
Rodin, Vadim Recent developments in calculations of nuclear double beta decay
Reliably calculated nuclear matrix elements M$^{0\nu}$ for the neutrinoless double beta decay are crucial for determining the absolute neutrino mass scale as well as for distinguishing between possible mechanisms of the decay (exchange of light and heavy neutrinos, SUSY particles, leptoquarks etc). In the talk, recent calculation results of different nuclear structure models are discussed. It is shown how an appropriate account of experimental data helps to drastically reduce uncertainties in the calculations of M$^{0\nu}$.
 
Roth, Robert Ab-Initio Nuclear Structure Calculations Beyond the p-Shell
The microscopic description of nuclei based on realistic nuclear interactions is a supreme challenge for nuclear structure theory. By starting from QCD-motivated realistic interactions one expects reliable predictions also for nuclei far off stability. These interactions, however, generate strong correlations in the nuclear many-body state, which cannot be described by simple many-body approximations. For p-shell nuclei, powerful ab initio tools like the No-Core Shell Model or the Green's Function Monte Carlo approach are available and have been employed successfully for nuclear structure studies. In this context I will review and compare different methods for deriving phase-shift equivalent effective interactions using unitary transformations, e.g. the Unitary Correlation Operator Method and the Similarity Renormalization Group. The extension of the domain of ab initio schemes to nuclei beyond the p-shell is crucial for future nuclear structure studies. I will discuss novel ideas to extend the range of reliable ab initio calculations towards intermediate-mass nuclei. Among those is an adaptive importance truncation of the no-core model space based on an a priori estimate for the relevance of individual basis states derived from perturbation theory. First applications reveal the quality and efficiency of these methods. They bridge the gap to approximate nuclear structure methods which, using the same effective interactions, give access to the whole nuclear chart.
 
Rubio Barroso, Berta  β-decay properties of Tz=-1 nuclei. Future experiments at FAIR DESPEC
We are now performing interesting experiments on the beta decay properties of Tz=-1 nuclei and its comparison with mirror transitions observed in charge exchange reactions. At the same time these series of experiments are used as a test bench for future experiments at FAIR and more particularly at DESPEC (Decay Spectroscopy) where I am the spokesperson. I think these topics nicely fit in your programme.
 
Sakurai, Hiroyoshi Nuclear Physics Programs with RIBF
I would like to show present status and coming programs at the new facility of RIBF, through introducing recent results obtained at the old facility.
 
Schnack, Jürgen Modern Aspects in Magnetic Structure and Dynamics
The physics of few-body quantum systems turns out to be rather universal. When changing from nuclei to magnetic molecules a lot of old friends as for instance highly correlated ground states, rotational modes (Yrast bands!) and phase transitions in small systems will be met again. In the talk I will introduce some of these concepts from a magnetic point of view. But there will of course be time left for some good old memories ...
 
Schuck, Peter Alpha-Particle Condensation in Nuclear Systems
It is now quite well established that at least the Hoyle state at 7.65 MeV in 12C has a wide extension where three alpha particles move almost independently, all in 0S-wave orbital, hold together only by the Coulomb barrier. It is very likely that analogous states exist in heavier nuclei around the alpha-disintegration threshold. First indications exist in 16O around 14 MeV. New theoretical results shall be presented. For increasing number of alpha-particles the Coulomb barrier fades away. Exciting 40Ca to the alpha-threshold of about 60MeV via a HIC an alpha coherent state with 10 alphas may be formed with a certain probability which starts expanding. Multiparticle detectors may identify the alphas. Experimental studies are under way at IPN Orsay. Alpha-particle condensation may exist in collapsing stars. The possibility of quartetting and quartet condensation in other systems like cold atoms shall be discussed.
 
Schury, Peter A Multi-Reflection Time-of-Flight Mass Spectrometer for Precision Mass Measurements of Very Short-Lived Nuclei
The understanding of halo-nuclei, the region near $^{42}$Si and the r-process pathway can be improved through precision mass measurements of nuclei with T$_{1/2}<$30 ms. Mass measurements of such very short-lived isotopes have thus far been limited to relativistic single-pass time-of-flight spectrometers such as SPEG at GANIL or the S800 at NSCL with typical relative mass uncertainties on the order of $\delta$m/m$\approx$10$^{-6}$. While Penning traps provide the highest possible mass precision, a low-energy multi-reflection time-of-flight (MRTOF) mass spectrograph provides a more versatile alternative. The RI Beam Factory (RIBF) at RIKEN will provide access to very neutron rich nuclei at unprecedented intensities. In order to perform precision mass measurements of these nuclei, an MRTOF mass spectrometer is under construction as part of the SLOWRI facility at RIKEN. The system is to be based on a small gas stopping cell and is designed to be portable, allowing a powerful degree of flexibility to maximize available on-line time for testing the device. By employing extremely highly stabilized voltage supplies, as well as an advanced ion preparation system, it is believed that relative precisions of $\delta$m/m$>$10$^{-7}$ can be obtained with a series of 3 ms measurements. Furthermore, such a system will be sufficiently sensitive to provide precise mass measurements of nuclei with production rates of perhaps as low as a few hundred per hour.
 
Schwenk, Achim Three-nucleon interactions and nuclear structure
 
 
Sorlin, Olivier Tensor and spin-orbit forces viewed from the study of the N=28 shell closure.
The N=28 shell closure is the first arising from the spin-orbit interaction. Its evolution in nuclei with large neutron to proton excesses is therefore potentially connected to that of the spin-orbit interaction. From the doubly magic 48Ca to the close to drip line 42Si nucleus, several structural modifications occur, starting from spherical, prolate-spherical co-existence to oblate shapes. Surprisingly a similar dramatic structural change does not occur for the N=20 isotones which remain remarkably spherical between the 40Ca and 34Si nuclei. By using up to date experimental data along the N=28 isotonic chain, such as (d,p) transfer reaction, in-beam gamma-ray spectroscopy, Coulomb excitation, isomeric transitions, the underlying physics origin for the profound structural modifications at the N=28 shell clsoure will be emphasized. Among these, the action of tensor forces and the central density dependence of the spin-orbit interaction will be commented.
 
Tanihata, Isao Spectroscopy of drip line nuclei with a thick target technique
The spectroscopy of exotic nuclei by transfer reactions has limitation due to the intensity of a RI beam. It requires a thick target to obtain a detectable amount of reaction first of all. However, in usual method, a thick target can not be used because of the energy loss of the low energy particles emitted from reactions. They either stop in the target or loose considerable amount of energies in the target and thus make the experiment impossible or the resolution too bad to separate individual states. Active target is one of the method to solve the problem. We show an experiment of 11Li(p,t)9Li reaction at TRIUMF using an active target MAYA. Also the extension of this method will be discussed for normal target geometry experiments.
 
Tsoneva Larionova, Nadezhda Pygmy Dipole Response in Exotic Nuclei in Multi-Phonon Representation.
Recently a theoretical method [1] incorporating HFB calculations of the nuclear ground states and the QPM theory was applied for investigations of low-energy dipole excitations in spherical N=50, N=82 isotones and the $Z=50$ [2] isotopes. The analysis of the corresponding neutron and proton dipole transition densities [2] in these nuclei allows to assign a genuine pattern to the low-energy dipole excitations - PDR modes and making them distinct from the conventional GDR modes. From calculations limited to the one-phonon QRPA approximation in all cases of N=50, N=82 and $^{110-132}$Sn nuclei (N$>$Z) a close connection between the total neutron PDR strengths and the neutron skin thickness defined by the relative difference of neutron and proton rms radii was found. An interesting observation is the most exotic $^{100}$Sn nucleus (N=Z), where at E*=8.3 MeV a state with a proton structure was found. This mode could be related to a proton PDR. Further development of the multi-phonon QPM theory is performed for the study of the fragmentation pattern of the low-energy dipole excitations, which can be achieved within a large model configuration space including up to three-phonon components. The reliable description of the experimental spectra is discussed and compared to recent data. [1] N. Tsoneva, H. Lenske, Ch. Stoyanov, Phys.\ Lett.\ {\bf B586} (2004) 213 and refs. therein. [2] N. Tsoneva, H. Lenske, arXiv:0706.4204Phys and refs. therein.
 
Typel, Stefan Pseudospin, Supersymmetry and the Shell Structure of Atomic Nuclei
The shell model is a cornerstone of nuclear structure physics since 50 years. Nucleons occupy single-particles states in a mean-field with strong central and spin-orbit components. The particular ordering in energy leads to the appearance of prominent shell gaps. Experimental observations suggest a change of the shell structure and the appearance of new magic numbers in exotic nuclei. The effects of the spin-orbit potential and the tensor interaction on the level structure have been discussed intensively in recent years. In fact, the slope of the single-particle energies can provide information on the monopole matrix elements of the effective interaction entering in shell model calculations. It is important to identify the contributions to the potential that are responsible for a change in the level structure. Single-particle levels defining the shell gaps are of particular interest. In most cases they belong to a pair of pseudospin partners that are almost degenerate in energy. A relativistic description seems to provide a natural explanation for this phenomenon. However, the symmetry-breaking potential in the relativistic explanation is not really a suitable tool in estimating the pseudospin breaking since it is not regular. An alternative description of the degeneracy is obtained by applying supersymmetric quantum mechanics. This approach is not limited to relativistic models and a regular symmetry breaking potential is obtained.
 
von Neumann-Cosel, Peter Electron Scattering as a Tool to Study Excited States with Unusual Features
I will discuss two examples of the power of high-resolution electron scattering spectroscopy to unravel unusual structures in light nuclei. The first case discusses the first excited state 1/2+ state in 9Be. It is unbound but just above the neutron trhreshold and thus shows an asymmetric line shape. Determining its resonance properties is of importance to estimate possible scenarios in supernovae, where 12C is produced in an alternative route to the Salpeter process via 9Be(alpha,n). At present there is a conflict in the literature on the correct resonance paremeters. I present new (e,e') experiments which resolve the problem. Furthermore the form factor is compared to NCSM calculations with large model spaces. The results indictae that this weak E1 transition might violate the Siegert theorem. The second part discusses the 0+ state at threshold in 12C (the Hoyle state). It is known to be of alpa-cluster structure, but recently it was claimed to possess a structure resembling a Bose-Einstein condensate. This claim is critically investigated through electron scattering, which provides information on the spatial structure of the Hoyle state.
 
Wolter, Hermann Low-density symmetry energy
The symmetry energy at densities from below saturation density down to very small values is important for the structure of exotic nuclei and for astrophysical processes like supernovae. I will discuss the results from attempts to gain information from heavy ion collisions at Fermi energies from isospin diffusion and migration. I will further discuss theoretical attemps to determine the low density EOS in the framework of RMF theory under contraints of neutron star observables, including many-body correlations at very low density and the formation of heavy nuclei in a neutron gas.
 
Zaryouni, Saeedeh nuclear matter with Skyrme potential
Nuclear matter is an idealized infinit uniform system of nucleons under their mutual strong interactins.The equation os state of nuclear and neutron matter has been studied by Skyrme porential at Zero temperature by by Hartree -Fock approximation.We have calculated asymetric energy and succeptibility of polarized neutron matter.The results are in good agreement with other methods and potentials.