Constraints on the Density Dependence of the Symmetry Energy
Joint Institute for Nuclear Astrophysics · National Superconducting Cyclotron Laboratory · +3 more institutions
Abstract
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.
Citation impact
- FWCI
- 86.02
- Percentile
- 100%
- References
- 30
Authors
7- MBM. B. TsangCorresponding
Joint Institute for Nuclear Astrophysics, National Superconducting Cyclotron Laboratory, Michigan State University
- YZYingxun Zhang
Joint Institute for Nuclear Astrophysics, Michigan State University, China Institute of Atomic Energy, National Superconducting Cyclotron Laboratory
- PDPaweł Danielewicz
Joint Institute for Nuclear Astrophysics, Michigan State University, National Superconducting Cyclotron Laboratory
- MFM. Famiano
Western Michigan University
- ZLZhuxia Li
China Institute of Atomic Energy
Topics & keywords
- Physics
- Symmetry (geometry)
- Observable
- Isospin
- Neutron
- Work (physics)
- Saturation (graph theory)
- Range (aeronautics)
- Affordable and clean energy