The physics of neutron star crusts is vast, involving many different research fields, from
nuclear and condensed matter physics to general relativity. This review summarizes the …

Neutron stars, the compact stellar remnants of core-collapse supernova explosions, are
unique cosmic laboratories for exploring novel phases of matter under extreme conditions …

The theory of the nuclear energy-density functional is used to provide a unified and
thermodynamically consistent treatment of all regions of cold non-accreting neutron stars. In …

We derive a new equation of state (EoS) for neutron stars (NS) from the outer crust to the
core based on modern microscopic calculations using the Argonne v 18 potential plus three …

Formed in the aftermath of gravitational core-collapse supernova explosions, neutron stars
are unique cosmic laboratories for probing the properties of matter under extreme conditions …

Even though the “free” neutrons in the inner crust of a neutron star are superfluid, they are
still strongly coupled to nuclei due to nondissipative entrainment effects. These effects have …

The equation of state (EoS) of hot and dense matter is a fundamental input to describe static
and dynamical properties of neutron stars, core-collapse supernovae and binary compact …

The equation of state and composition of the inner crust of neutron stars at zero temperature
are calculated, using the T= 0 version of the temperature-dependent extended Thomas …

We generalize our earlier work on neutron stars, which assumed spherical Wigner-Seitz
cells in the inner crust, to admit the possibility of pasta phases, ie, nonspherical cell shapes …

We present a systematic survey of the range of predictions of the neutron star inner crust
composition, crust-core transition densities and pressures, and density range of the nuclear" …