Probing the symmetry energy at high baryon density with heavy ion collisions

TL;DR

This paper discusses how heavy ion collisions at high energies can be used to probe the poorly understood nuclear symmetry energy at high densities, emphasizing the importance of including momentum dependence and isospin effects in models.

Contribution

It highlights key observables and physical mechanisms necessary for constraining the symmetry energy through experimental data and theoretical modeling.

Findings

Identifies observables like $n/p$ emission and meson yield ratios for symmetry energy constraints.

Emphasizes the importance of including momentum dependence of isospin fields in models.

Discusses upcoming experiments capable of distinguishing isospin effects.

Abstract

The nuclear symmetry energy at densities above saturation density ($\rho_0\sim 0.16 fm^{-3}$) is poorly constrained theoretically and very few relevant experimental data exist. Its study is possible through Heavy Ion Collisions (HIC) at energies $E/A> 200$ MeV, particularly with beams of neutron-rich radioactive nuclei. The energy range implies that the momentum dependence of the isospin fields, i.e. the difference of the effective masses on protons and neutrons, also has to be investigated before a safe constraint on $\esy(\rho)$ is possible. We discuss the several observables which have been suggested, like $n/p$ emission and their collective flows and the ratio of meson yields with different isospin projection, $\pi^-/\pi^+$ and $K^0/K^+$. We point out several physical mechanisms that should be included in the theoretical models to allow a direct comparison to the more precise experiments which will be able to distinguish the isospin projection of the detected particles: CSR/Lanzhou, FAIR/GSI, RIBF/RIKEN, FRIB/MSU.