Influence of the treatment of initialization and mean-field potential on the neutron to proton yield ratios
arXiv:2103.13132 · doi:10.1103/PhysRevC.104.024605
Abstract
In this work, we firstly investigate how to reproduce and how well one can reproduce the Woods-Saxon density distribution of initial nuclei in the framework of the improved quantum molecular dynamics model. Then, we propose a new treatment for the initialization of nuclei which is correlated with the nucleonic mean-field potential by using the same potential energy density functional. In the mean field potential, the three-body force term is accurately calculated. Based on the new version of the model, the influences of precise calculations of the three-body force term, the slope of symmetry energy, the neutron-proton effective mass splitting, and the width of the wave packet on heavy ion collision observables, such as the neutron to proton yield ratios for emitted free nucleons [] and for coalescence invariant nucleons [] for Sn+Sn at the beam energy of 200 MeV per nucleon, are discussed. Our calculations show that the spectra of neutron to proton yield ratios [] can be used to probe the slope of symmetry energy () and the neutron-proton effective mass splitting. In detail, the in the low kinetic energy region can be used to probe the slope of symmetry energy (). With a given , the inclination of to kinetic energy () can be used to probe the effective mass splitting. In the case where the neutron-proton effective mass splitting is fixed, at high kinetic energy can also be used to learn the symmetry energy at suprasaturation density.
arXiv comment8 pages, 4 figures
References in corpus (43)
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- GW170817: Measurements of Neutron Star Radii and Equation of State
- Microscopic Models for Ultrarelativistic Heavy Ion Collisions
- Recent Progress and New Challenges in Isospin Physics with Heavy-Ion Reactions
- Properties of the binary neutron star merger GW170817
- Gravitational-wave constraints on the neutron-star-matter Equation of State
- Constraints on the symmetry energy and neutron skins from experiments and theory
- Reaction Dynamics with Exotic Beams
- Constraints on the density dependence of the symmetry energy
- Skyrme Interaction and Nuclear Matter Constraints
- Nuclear symmetry energy probed by neutron skin thickness of nuclei
- Determination of the stiffness of the nuclear symmetry energy from isospin diffusion
- Neutron skins and neutron stars in the multi-messenger era
- Analysis of the (N,xN') reactions by quantum molecular dynamics plus statistical decay model
- Density slope of the nuclear symmetry energy from the neutron skin thickness of heavy nuclei
- Symmetry Energy II: Isobaric Analog States
- Probing the High Density Behaviour of Nuclear Symmetry Energy with High Energy Heavy-Ion Collisions
- Results of the ASY-EOS experiment at GSI: The symmetry energy at suprasaturation density
- Equation of state of asymmetric nuclear matter and collisions of neutron-rich nuclei
- Neutron and Proton Transverse Emission Ratio Measurements and the Density Dependence of the Asymmetry Term of the Nuclear Equation of State
- Understanding transport simulations of heavy-ion collisions at 100 and 400 AMeV: Comparison of heavy ion transport codes under controlled conditions
- Parton-Hadron-Quantum-Molecular Dynamics (PHQMD) -- A Novel Microscopic N-Body Transport Approach for Heavy-Ion Collisions, Dynamical Cluster Formation and Hypernuclei Production
- Elliptic flow and system size dependence of transition energies at intermediate energies
- The influence of cluster emission and the symmetry energy on neutron-proton spectral double ratios
- Towards a model-independent constraint of the high-density dependence of the symmetry energy
- Nuclear symmetry energy at subnormal densities from measured nuclear masses
- Momentum dependence of the symmetry potential and its influence on nuclear reactions
- Probing the density dependence of the symmetry potential at low and high densities
- Constraints on symmetry energy and nucleon effective mass splitting with Heavy Ion Collisions
- Constraints on the symmetry energy and its associated parameters from nuclei to neutron stars
- Feasability of constraining the curvature parameter of the symmetry energy using elliptic flow data
- Insights on Skyrme parameters from GW170817
- Progress of Quantum Molecular Dynamics model and its applications in Heavy Ion Collisions
- Delineating Effects of Nuclear Symmetry Energy on the Radii and Tidal Polarizabilities of Neutron Stars
- Symmetry energy constraints from GW170817 and laboratory experiments
- Nuclear symmetry energy from the Fermi-energy difference in nuclei
- Triton-He relative and differential flows as probes of the nuclear symmetry energy at supra-saturation densities
- Tides in merging neutron stars: Consistency of the GW170817 event with experimental data on finite nuclei
- Influence of neutron-skin thickness on ratio in Pb+Pb collisions
- Insights on pion production mechanism and symmetry energy at high density
- Revisit of the neutron/proton ratio puzzle in intermediate-energy heavy-ion collisions
- Competition between Coulomb and Symmetry Potential in Semi-peripheral Heavy-ion Collisions
- The influence of the neutron skin and the asymmetry energy on the ratio
Cited by in corpus (4)
- Comparison of Heavy-Ion Transport Simulations: Mean-field Dynamics in a Box
- Isovector giant dipole resonance mode with an improved propagation approach in the framework of EQMD model
- A novel filtering method for generating desired density profiles of colliding nuclei
- Covariant formulation of relativistic quantum molecular dynamics for a system of interacting wave packets