Neutrinos are known to play important roles in many astrophysical scenarios from the early
period of the big bang to current stellar evolution being a unique messenger of the fusion …

Nuclear pasta, with nonspherical shapes, is expected near the base of the crust in neutron
stars. Large-scale molecular dynamics simulations of pasta show long lived topological …

A neutron star was first detected as a pulsar in 1967. It is one of the most mysterious
compact objects in the universe, with a radius of the order of 10 km and masses that can …

Complex and exotic nuclear geometries, collectively referred to as “nuclear pasta,” are
expected to appear naturally in dense nuclear matter found in the crusts of neutron stars and …

We analyze different stages of magnetized quark star evolution incorporating baryon
number conservation and using an anisotropic energy–momentum tensor. The first stages of …

The presence of nuclear pasta is expected to modify the transport properties in the mantle of
neutron stars. The non-spherical geometry of the pasta nuclear clusters leads to …

We present a minimal nuclear energy density functional (NEDF) called “SeaLL1” that has
the smallest number of possible phenomenological parameters to date. SeaLL1 is defined …

Background: The dense neutron-rich matter found in supernovae and inside neutron stars is
expected to form complex nonuniform phases, often referred to as nuclear pasta. The pasta …

Nuclear pasta topology is an essential ingredient to determine transport properties in the
inner crust of neutron stars. We perform semiclassical molecular dynamics simulations of …

We investigate the existence of possible stable strange matter and related stability windows
at finite temperature for different models that are generally applied to describe quark stars …