Using a meta model for nuclear Equation of State (EOS) with its parameters constrained by
astrophysical observations and terrestrial nuclear experiments, we examine effects of …

Magnetic fields are ubiquitous across different physical systems of current interest; from the
early Universe, compact astrophysical objects and heavy-ion collisions to condensed matter …

We study consistently the effects of magnetic field on hot and dense matter. In particular, we
look for differences that arise due to assumptions that reproduce the conditions produced in …

In the present work, we consider nuclear matter in the innermost crust of neutron stars under
the presence of a strong magnetic field within the framework of a relativistic mean-field …

The neutrino mean free path is evaluated in hot proto–neutron star matter under a strong
magnetic field. We consider densities in the range 0.04≤ ρ≤ 0.4 fm− 3, several proton …

In recent years, the impact of strong magnetic fields on the strongly interacting matter phase
diagram has been a very active field of research with important developments. The presence …

Using a meta model for nuclear Equation of State (EOS) with its parameters constrained by
astrophysical observations and terrestrial nuclear experiments, we examine effects of …

We study the properties of hot and dense neutron star matter under the presence of strong
magnetic fields using two Skyrme interactions, namely the LNS and the BSk21 ones. Asking …