Symmetry potentials and in-medium nucleon-nucleon cross sections within the Nambu-Jona-Lasinio model in relativistic impulse approximation

TL;DR

This study compares symmetry potentials and in-medium nucleon-nucleon cross sections derived from the NJL and RMF models within the relativistic impulse approximation, highlighting the effects of chiral symmetry restoration at high densities.

Contribution

It introduces the use of the NJL model to analyze symmetry potentials and NN cross sections, emphasizing chiral symmetry effects beyond saturation density.

Findings

Symmetry potentials rise significantly with density in the NJL model.

In-medium NN cross sections increase with density, sharply in the NJL model during chiral symmetry restoration.

NJL model exhibits distinct energy-dependent behaviors compared to RMF models.

Abstract

In the relativistic impulse approximation (RIA), we study symmetry potentials and in-medium nucleon-nucleon (NN) cross sections with the Nambu-Jona-Lasinio (NJL) model that features chiral symmetry. The chiral symmetry that plays a fundamental role in the nonperturbative physics in the strong interaction is anticipated to add restrictive effects on the symmetry potentials and in-medium NN cross sections. For comparison, we also perform the study with the usual relativistic mean-field (RMF) model. The numerical results with the NJL and RMF models are similar at saturation density and below, since a priori fit was made to saturation properties. With the increase of nuclear density, the chiral symmetry starts to be restored partially in the NJL model, resulting in the explicit fall of the scalar density. In a large energy span, the symmetry potential acquires a significant rise for the partial restoration of the chiral symmetry, compared to the one with the RMF model. It is found that the in-medium NN cross sections in the RIA with the NJL and RMF models both increase with the density in the energy region interested in this study, whereas those with the NJL model increase sharply as long as a clear chiral symmetry restoration takes place. The different tendency of observables in density can be transmitted to the different energy dependence in the RIA. The NJL model is shown to have characteristic energy-dependent symmetry potentials and NN cross sections beyond saturation point, apart from the RMF models.