The ultimate goal of studying isospin physics via heavy-ion reactions with neutron-rich,
stable and/or radioactive nuclei is to explore the isospin dependence of in-medium nuclear …

In this review we study the nuclear pastas as they are expected to be formed in neutron star
crusts. We start with a study of the pastas formed in nuclear matter (composed of protons …

The density dependence of the symmetry energy in the equation of state of isospin
asymmetric nuclear matter is of significant importance for studying the structure of systems …

Neutron star crusts are studied using a classical molecular dynamics model developed for
heavy-ion reactions. After the model is shown to produce a plethora of the so-called pasta …

The single-particle potential for nucleons and hyperons in neutron-rich matter generally
depends on the density and isospin asymmetry of the medium as well as the momentum and …

Within a self-consistent thermal model using an isospin and momentum dependent
interaction (MDI) constrained by the isospin diffusion data in heavy-ion collisions, we …

Experimental information on fragment emissions is important in understanding the dynamics
of nuclear collisions and in the development of transport model simulating heavy-ion …

The ratio of the symmetry energy coefficient to temperature, a sym/T, in Fermi energy heavy-
ion collisions, was experimentally extracted as a function of the fragment atomic number …

In this work, we focus on different length scales within the dynamics of nucleons in
conditions according to the neutron star crust, with a semiclassical molecular dynamics …

Ideal nuclear matter is expected to undergo a first order phase transition at the
thermodynamic limit. At such phase transitions the size of density fluctuations (bubbles or …