AbstractUsing covariance analysis, we quantify the correlations between the interaction parameters in a transport model and the observables commonly used to extract information of the Equation of State of Asymmetric Nuclear Matter in experiments. By simulating 124Sn + 124Sn, 124Sn + 112Sn and 112Sn + 112Sn reactions at beam energies of 50 and 120 MeV per nucleon, we have identified that the nucleon effective mass splitting is most strongly correlated to the neutrons and protons yield ratios with high kinetic energy from central collisions especially at high incident energy. The best observable to determine the slope of the symmetry energy, L, at saturation density is the isospin diffusion observable even though the correlation is not very s...
The symmetry energy is the energy difference between symmetric nuclear matter and pure neutron matte...
Heavy Ion Collisions (HIC) represent a unique tool to probe the in-medium nuclear interaction in reg...
The N/Z ratio of free nucleons from collisions of neutron-rich nuclei as a function of their momentu...
Using covariance analysis, we quantify the correlations between the interaction parameters in a tran...
Using covariance analysis, we quantify the correlations between the interaction parameters in a tran...
AbstractUsing covariance analysis, we quantify the correlations between the interaction parameters i...
Using covariance analysis, we quantify the correlations between the interaction parameters in a tran...
A new version of the improved quantum molecular dynamics model has been developed to include standar...
AbstractA new version of the improved quantum molecular dynamics model has been developed to include...
The density dependence of the symmetry energy in the equation of state of asymmetric nuclear matter ...
The nuclear equation of state is a topic of highest current interest in nuclear structure and reacti...
The role of isospin asymmetry in nuclei and neutron stars is discussed, with an emphasis on the dens...
The role of isospin asymmetry in nuclei and neutron stars is discussed, with an emphasis on the dens...
The role of isospin asymmetry in nuclei and neutron stars is discussed, with an emphasis on the dens...
The role of isospin asymmetry in nuclei and neutron stars is discussed, with an emphasis on the dens...
The symmetry energy is the energy difference between symmetric nuclear matter and pure neutron matte...
Heavy Ion Collisions (HIC) represent a unique tool to probe the in-medium nuclear interaction in reg...
The N/Z ratio of free nucleons from collisions of neutron-rich nuclei as a function of their momentu...
Using covariance analysis, we quantify the correlations between the interaction parameters in a tran...
Using covariance analysis, we quantify the correlations between the interaction parameters in a tran...
AbstractUsing covariance analysis, we quantify the correlations between the interaction parameters i...
Using covariance analysis, we quantify the correlations between the interaction parameters in a tran...
A new version of the improved quantum molecular dynamics model has been developed to include standar...
AbstractA new version of the improved quantum molecular dynamics model has been developed to include...
The density dependence of the symmetry energy in the equation of state of asymmetric nuclear matter ...
The nuclear equation of state is a topic of highest current interest in nuclear structure and reacti...
The role of isospin asymmetry in nuclei and neutron stars is discussed, with an emphasis on the dens...
The role of isospin asymmetry in nuclei and neutron stars is discussed, with an emphasis on the dens...
The role of isospin asymmetry in nuclei and neutron stars is discussed, with an emphasis on the dens...
The role of isospin asymmetry in nuclei and neutron stars is discussed, with an emphasis on the dens...
The symmetry energy is the energy difference between symmetric nuclear matter and pure neutron matte...
Heavy Ion Collisions (HIC) represent a unique tool to probe the in-medium nuclear interaction in reg...
The N/Z ratio of free nucleons from collisions of neutron-rich nuclei as a function of their momentu...