We review the current status and recent progress of microscopic many-body approaches
and phenomenological models, which are employed to construct the equation of state of …

A review is given of various theoretical approaches for the equation of state (EoS) of dense
matter, relevant for the description of core-collapse supernovae, compact stars, and compact …

The understanding of stellar structure represents the crossroads of our theories of the
nuclear force and the gravitational interaction under the most extreme conditions observably …

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 …

Our family of three Hartree-Fock-Bogoliubov (HFB) mass models, labeled BSk19, BSk20,
and BSk21, is here extended by (a) refitting to the 2012 Atomic Mass Evaluation (AME), and …

The gravitational wave signal from a binary neutron star inspiral contains information on the
nuclear equation of state. This information is contained in a combination of the tidal …

Context. An equation of state (EoS) of dense nuclear matter is a prerequisite for studies of
the structure and evolution of compact stars. A unified EoS should describe the crust and the …

Abstract Recently, the Canadian Hydrogen Intensity Mapping Experiment detected
periodicity in the bursting rate of the repeating FRB 180916. J0158+ 65. In a popular class of …

Large pulsar frequency glitches are generally interpreted as sudden transfers of angular
momentum between the neutron superfluid permeating the inner crust and the rest of the …

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 …