Collisions involving {112Sn} and {124Sn} nuclei have been simulated with the improved quantum molecular dynamics transport model. The results of the calculations reproduce isospin diffusion data from two different observables and the ratios of neutron and proton spectra. By comparing these data to calculations performed over a range of symmetry energies at saturation density and different representations of the density dependence of the symmetry energy, constraints on the density dependence of the symmetry energy at subnormal density are obtained. The results from the present work are compared to constraints put forward in other recent analyses.

1 aTsang, M., B.1 aZhang, Yingxun1 aDanielewicz, P.1 aFamiano, M.1 aLi, Z.1 aLynch, W., G.1 aSteiner, A., W. uhttps://icer.msu.edu/research/publications/constraints-density-dependence-symmetry-energy01591nas a2200217 4500008004100000245007600041210006900117260001200186300001100198490000800209520092200217100001801139700001501157700001501172700001601187700001401203700001201217700001801229700001501247856011101262 2009 eng d00aSurvey of Excited State Neutron Spectroscopic Factors for Z=8-28 Nuclei0 aSurvey of Excited State Neutron Spectroscopic Factors for Z828 N c01/2009 a0625010 v1023 aWe have extracted 565 neutron spectroscopic factors of sd and fp shell nuclei by systematically analyzing more than 2000 measured (d, p) angular distributions. We are able to compare 125 of the extracted spectroscopic factors to values predicted by large-basis shell-model calculations and evaluate the accuracies of spectroscopic factors predicted by different shell-model interactions in these regions. We find that the spectroscopic factors predicted for most excited states of sd-shell nuclei using the latest {USDA} or {USDB} interactions agree with the experimental values. For fp shell nuclei, the inability of the current models to account for the core excitation and fragmentation of the states leads to considerable discrepancies. In particular, the agreement between data and shell-model predictions for Ni isotopes is not better than a factor of 2 using either the {GXPF1A} or the {XT} interaction.

1 aTsang, M., B.1 aLee, Jenny1 aSu, S., C.1 aDai, J., Y.1 aHoroi, M.1 aLiu, H.1 aLynch, W., G.1 aWarren, S. uhttps://icer.msu.edu/research/publications/survey-excited-state-neutron-spectroscopic-factors-z8-28-nuclei01478nas a2200193 4500008004100000245010300041210006900144260001200213300001400225490000800239520081400247100001901061700002001080700001601100700001101116700001801127700001801145856012101163 2008 eng d00aThe influence of cluster emission and the symmetry energy on neutron-proton spectral double ratios0 ainfluence of cluster emission and the symmetry energy on neutron c02/2008 a145–1480 v6643 aThe emissions of neutrons, protons and bound clusters from central {124Sn} + {124Sn} and {112Sn} + {112Sn} collisions are simulated using the Improved Quantum Molecular Dynamics model for two different density-dependent symmetry-energy functions. The calculated neutron-proton spectral double ratios for these two systems are sensitive to the density dependence of the symmetry energy, consistent with previous work. Cluster emission increases the double ratios in the low energy region relative to values calculated in a coalescence-invariant approach. To circumvent uncertainties in cluster production and secondary decays, it is important to have more accurate measurements of the neutron-proton ratios at higher energies in the center of mass system, where the influence of such effects is reduced.

1 aZhang, Yingxun1 aDanielewicz, P.1 aFamiano, M.1 aLi, Z.1 aLynch, W., G.1 aTsang, M., B. uhttps://icer.msu.edu/research/publications/influence-cluster-emission-symmetry-energy-neutron-proton-spectral-double01816nas a2200217 4500008004100000245009100041210006900132260001200201490000700213520109300220653002301313653001901336100001401355700001801369700001601387700001201403700002001415700001801435700001901453856012601472 2008 eng d00aTransport Model Simulations of Projectile Fragmentation Reactions at 140 {MeV/nucleon}0 aTransport Model Simulations of Projectile Fragmentation Reaction c08/20080 v783 aThe collisions in four different reaction systems using {\$ˆ{40,48}\$Ca} and {\$ˆ{58,64}\$Ni} isotope beams and a Be target have been simulated using the Heavy Ion Phase Space Exploration and the Antisymmetrized Molecular Dynamics models. The present study mainly focuses on the model predictions for the excitation energies of the hot fragments and the cross sections of the final fragments produced in these reactions. The effects of various factors influencing the final fragment cross sections, such as the choice of the statistical decay code and its parameters have been explored. The predicted fragment cross sections are compared to the projectile fragmentation cross sections measured with the A1900 mass separator. At {\$E/A=140\$} {MeV,} reaction dynamics can significantly modify the detection efficiencies for the fragments and make them different from the efficiencies applied to the measured data reported in the previous work. The effects of efficiency corrections on the validation of event generator codes are discussed in the context of the two models.

10aNuclear Experiment10aNuclear Theory1 aMocko, M.1 aTsang, M., B.1 aLacroix, D.1 aOno, A.1 aDanielewicz, P.1 aLynch, W., G.1 aCharity, R., J uhttps://icer.msu.edu/research/publications/transport-model-simulations-projectile-fragmentation-reactions-140-mev-nucleon